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SpACe-Time pRoCeSSing AppliCATionS foR wiReleSS CommuniCATionS

2008

Wireless mobile communication networks are rapidly growing at an incredible rate around the world and a number of improved and emerging technologies are seen to be critical to the improved economics and performance of these networks. The technical revolution and continuing growth of mobile radio communication systems has been made possible by extraordinary advances in the related fields of digital computing, highspeed circuit technology, the Internet and, of course, digital signal processing. Improved third generation (3G) and future generation wireless communication systems must support a substantially wider and enhanced range of services with respect to those supported by second generation and basic 3G systems. The never-ending quest for such personal and multimedia services, however, demands technologies operating at higher data rates and broader bandwidths. This combined with the unpredictability and randomness of the mobile propagation channel has created many new technically challenging problems for which innovative, adaptive and advanced signal processing techniques may offer new and better solutions. Space-time processing techniques have emerged as one of the most promising areas of research and development in wireless communications for the efficient utilization of the physical mobile radio propagation channel. Space-time processing signifies the signal processing performed on a system consisting of several antenna elements, whose signals are processed adaptively in order to exploit both the spatial (space) and temporal (time) dimensions of the radio channel. This can significantly improve the capacity, coverage, quality and energy efficiency of wireless systems. This thesis expands the scope of space-time processing by proposing novel applications in wireless communication systems. These include the reduction of possibly harmful electromagnetic radiation from mobile phones, enhancing the quality of Bluetooth links in indoor office environments, increasing the spectral efficiency of satellite and the novel high altitude platforms (HAPs) communication systems, enhancing the coverage and capacity of integrated multiple-HAP 3G systems, and improving the energy efficiency of cooperative wireless sensor networks. The performance of these systems is assessed by theoretical analysis, by computer simulations under a range of propagation environments including realistic channel models, advanced commercial electromagnetic modeling software, and a proposed novel multichannel simulator suitable for various space-time applications. space-time processing applications for wireless communications ABSTRACT Tommy Hult ISSN 1653-2090 ISBN 978-91-7295-146-4 2008:12 2008:12 space-time processing applications for wireless communications Tommy Hult Blekinge Institute of Technology Doctoral Dissertation Series No. 2008:12 School of Engineering Space-Time Processing Applications for Wireless Communications Tommy Hult Blekinge Institute of Technology Doctoral Dissertation Series No 2008:12 ISSN 1653-2090 ISBN 978-91-7295-146-4 Space-Time Processing Applications for Wireless Communications Tommy Hult Department of Signal Processing School of Engineering Blekinge Institute of Technology SWEDEN © 2008 Tommy Hult Department of Signal Processing School of Engineering Publisher: Blekinge Institute of Technology Printed by Printfabriken, Karlskrona, Sweden 2008 ISBN 978-91-7295-146-4 ABSTRACT Wireless mobile communication networks are rapidly growing at an incredible rate around the world and a number of improved and emerging technologies are seen to be critical to the improved economics and performance of these networks. The technical revolution and continuing growth of mobile radio communication systems has been made possible by extraordinary advances in the related fields of digital computing, high-speed circuit technology, the Internet and, of course, digital signal processing. Improved third generation (3G) and future generation wireless communication systems must support a substantially wider and enhanced range of services with respect to those supported by second generation and basic 3G systems. The never-ending quest for such personal and multimedia services, however, demands technologies operating at higher data rates and broader bandwidths. This combined with the unpredictability and randomness of the mobile propagation channel has created many new technically challenging problems for which innovative, adaptive and advanced signal processing techniques may offer new and better solutions. Space-time processing techniques have emerged as one of the most promising areas of research and development in wireless communications for the efficient utilization of the physical mobile radio propagation channel. Space-time processing signifies the signal processing performed on a system consisting of several antenna elements, whose signals are processed adaptively in order to exploit both the spatial (space) and temporal (time) dimensions of the radio channel. This can significantly improve the capacity, coverage, quality and energy efficiency of wireless systems. This thesis expands the scope of space-time processing by proposing novel applications in wireless communication systems. These include the reduction of possibly harmful electromagnetic radiation from mobile phones, enhancing the quality of vi Bluetooth links in indoor office environments, increasing the spectral efficiency of satellite and the novel high altitude platforms (HAPs) communication systems, enhancing the coverage and capacity of integrated multiple-HAP 3G systems, and improving the energy efficiency of cooperative wireless sensor networks. The performance of these systems is assessed by theoretical analysis, by computer simulations under a range of propagation environments including realistic channel models, advanced commercial electromagnetic modeling software, and a proposed novel multichannel simulator suitable for various space-time applications. vii Acknowledgments I would like to express my sincere gratitude to Professor Ingvar Claesson for giving me the opportunity to be a Ph.D student at Blekinge Institute of Technology. I am utterly grateful and indebted to my supervisor and very good friend Professor Abbas Mohammed without whose help, insight, experience and nice discussions this thesis would not exist. I would also like to thank M.Sc. Zhe Yang and Dr. Ronnie Landqvist for the nice discussions and friendship during this time. Further I would like to thank all the collegues and friends at the Department. Special thanks to Dr. David Grace at University of York for letting me visit his group and for our nice collaborations within the EU COST 297 Action. I would also like to thank Professor Sven Nordebo, who suggested the possibility to continue as a Ph.D student after my Master thesis. Finally, I would like to thank my parents Kjell and Marianne, my sister LiseLotte, her husband Patrik and their children Axel and Elin for supporting me during these years. Tommy Hult Ronneby, September 2008. CONTENTS List of Publications Abbrevations and Acronyms Symbols and Notations 1 Introduction 1.1 Outline of the Thesis and Contributions . . . . . . . . 2 A Novel Space-Time-Polarization Channel Model for Wireless Communications 2.1 Space-Time-Polarization Channel Model . 2.1.1 Space-Polarization Channel Model 2.1.2 Statistical properties of the global channel matrix . . . . . . . . 2.1.3 Numerical Implementation . . . . . 2.2 Simulation Results . . . . . . . . . . . . . . . 2.3 Conclusions . . . . . . . . . . . . . . . . . . . 3 21 22 . . . . . . . . . . . . 27 28 29 . . . . . . . . 35 39 41 47 Space-Time-Polarization Processing for Capacity Enhancement in HAP/Satellite communication systems 3.1 Platform Diversity . . . . . . . . . . . . . . . . . . . . . 49 51 . . . . . . . . . . . . . . . . x 3.2 3.3 3.4 3.5 3.6 4 5 6 3.1.1 Space-Polarization Channel Model . . . . The MIMO-OFDM System . . . . . . . . . . . . . Compact Antenna Arrays . . . . . . . . . . . . . . 3.3.1 Array Configurations . . . . . . . . . . . . . 3.3.2 The Space-Polarization Domain . . . . . . 3.3.3 Mutual Coupling and Spatial Correlation Depolarization Analysis . . . . . . . . . . . . . . . . Simulation Results . . . . . . . . . . . . . . . . . . . Conclusions . . . . . . . . . . . . . . . . . . . . . . . Space-Time Processing for Quality Improvement of Short Range Wireless Communication Links 4.1 The Tested Indoor Office Environment . . . 4.1.1 The Used Antennas . . . . . . . . . . 4.1.2 The Measurements Setup . . . . . . . 4.2 Results of the Measurements . . . . . . . . . 4.3 FEM Simulations . . . . . . . . . . . . . . . . 4.3.1 The Simulated Indoor Model . . . . . 4.3.2 FEM Simulation Results . . . . . . . . 4.4 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56 57 59 59 59 70 71 72 84 . . . . . . . . . . . . . . . . 85 87 87 90 91 95 95 97 111 Power Constrained Space-Time Processing for Suppression of Electromagnetic Fields 5.1 The Model . . . . . . . . . . . . . . . . . . . . . . . . . 5.1.1 The FEM model . . . . . . . . . . . . . . . . . 5.1.2 The MIMO model . . . . . . . . . . . . . . . . 5.2 The Adaptive Algorithms . . . . . . . . . . . . . . . . 5.3 Simulation Results . . . . . . . . . . . . . . . . . . . . . 5.4 Power Constraints . . . . . . . . . . . . . . . . . . . . . 5.5 The Effects of MIMO Antenna Parameters and Carrier Frequency . . . . . . . . . . . . . . . . . . . . . . . 5.6 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . Space-Time Processing for Interference Mitigation in HAP WCDMA Systems 6.1 Multiple HAP system setup . . . . . . . 6.1.1 User Positioning Geometry . . . 6.1.2 Base station antenna pattern . . 6.1.3 User equipment antenna pattern . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 113 115 115 120 125 130 133 137 139 151 153 154 154 155 xi 6.2 6.3 6.4 7 8 6.1.4 UE-HAP radio propagation channel 6.1.5 WCDMA Setup . . . . . . . . . . . . 6.1.6 Space-Time Processing Techniques Interference analysis . . . . . . . . . . . . . . Simulation Results . . . . . . . . . . . . . . . Conclusions . . . . . . . . . . . . . . . . . . . Cooperative Space-Time Processing for Power Efficient Wireless Sensor Networks 7.1 Cooperative Beamforming . . . . . . . 7.2 Spatial Diversity Techniques . . . . . . 7.2.1 Cooperative MISO and SIMO 7.2.2 Cooperative MIMO . . . . . . 7.3 Simulation Results . . . . . . . . . . . . 7.4 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156 157 157 159 161 167 . . . . . . . . . . . . 169 170 173 175 177 178 180 . . . . . . . . . . . . . . . . . . . . . . . . Conclusions Appendix 181 A A Spherical Vector Harmonics A.1 Spherical Vector Harmonics . . . . . . . . . . . . . . . 185 187 B Antenna Types B.1 Antenna types . . . . . . . . . . . . . . . . . . . . . . . 189 191 C WCDMA Power Control C.1 WCDMA Power Control . . . . . . . . . . . . . . . . . 193 195 D Beamforming D.1 Beamforming . . . . . . . . . . . . . . . . . . . . . . . . 197 199 11 List of Publications Parts of Chapter 2 is published as: T. Hult, A. Mohammed, Theoretical Analysis and Assessment of Depolarization Effects on the Performance of High Altitude Platforms, COST 297 HAPCOS meeting and workshop, Nicosia, Cyprus, 7-9 April 2008. T. Hult, E. Falletti, A. Mohammed, F. Sellone, Multi-Antenna Multi-HAP Channel Model for Space-Polarization, COST 297 - HAPCOS meeting and workshop, Nicosia, Cyprus, 7-9 April 2008. T. Hult, E. Falletti, A. Mohammed, F. Sellone, Multi-channel model for spacepolarization systems, European Union Conference on Antennas and Propagation, EUCAP2007, Edinburgh, UK, 11-16 November 2007. T. Hult, A. Mohammed, E. Falletti, F. Sellone, Analysis of Depolarizing Effects and Impact on the Performance of a Multiple Satellite System Employing Polarization Diversity, International Union of Radio Science (URSI 2007), Ottawa, Canada, July 22-26 2007. Z. Yang, A. Mohammed, O. Awoniyi, A.O. Oladipo, T. Hult, M. Salomonsson, Comparative Analysis of Channel Models for Stratospheric Propagation, 2nd International Conference on Experiments/Process/System Modelling/Simulation&Optimization (IC-EpsMso), Athens, Greece, 2007. T. Hult, E. Falletti, A. Mohammed and F. Sellone, The Impact of Depolarizing Effects on a Multiple HAP System Employing Polarization Diversity, International Union of Radio Science (URSI 2007), Ottawa, Canada, July 22-26 2007. A. Mohammed and T. Hult, Evaluation of Depolarization Effects on the Performance of High Altitude Platforms (HAPs), IEEE 67th Vehicular Technology Conference, Marina Bay, Singapore, 11-14 May, 2008. 12 Parts of Chapter 3 is published as: T. Hult, A. Mohammed, Z. Yang and D. Grace; Performance of a Multiple HAP System Employing Multiple Polarization, Wireless Personal Communications Journal, Springer, Invited Paper, Special Issue, Journal No. 11277, Article No. 9511, 2008. A. Mohammed and T. Hult, Evaluation of Depolarization Effects on the Performance of High Altitude Platforms (HAPs), IEEE 67th Vehicular Technology Conference, Marina Bay, Singapore, 11 - 14 May, 2008. T. Hult, E. Falletti, A. Mohammed and F. Sellone; Multi-Antenna MultiHAP Channel Model for Space-Polarization, COST 297 - HAPCOS meeting and workshop, Nicosia, Cyprus, 7-9 April, 2008. T. Hult, E. Falletti, A. Mohammed and F. Sellone; The Impact of Depolarizing Effects on a Multiple HAP System Employing Polarization Diversity, International Union of Radio Science, URSI 2007, Ottawa, Canada, 22-26 July, 2007. T. Hult and A. Mohammed; Assessment of a HAP Diversity System Employing Compact MIMO-Tetrahedron Antenna, COST 297 - meeting and workshop, Prague, Czech Republic, 29-30 March, 2007. T. Hult and A. Mohammed; Compact MIMO Antennas and HAP Diversity for Enhanced Data Rate Communications, IEEE 65th Semiannual Vehicular Technology Conference, Dublin, Ireland, 22 - 25 April, 2007. A. Mohammed and T.Hult; Compact MIMO Antennas and Satellite Diversity for High Data Rate Communications, 8th annual IEEE Wireless and Microwave Technology, WAMICON06, Clearwater, USA, 4-5 December, 2006. T. Hult and A. Mohammed; Capacity of multiple hap system employing multiple polarizations, European Union Conference on Antennas and Propagation, EUCAP2006, Nice, France, 6-9 November, 2006. T. Hult and A. Mohammed; Capacity of a Satellite Diversity System Employing Multiple Polarizations, European Union Conference on Antennas and Propagation, EUCAP2006, Nice, France, 6-9 November, 2006. 13 T. Hult and A. Mohammed; Multiple HAP and Polarization Diversity for Enhanced Data Rate Communications, COST 297 - HAPCOS meeting YORK HAPWEEK workshop, York, UK, 26-27 October, 2006. T. Hult and A. Mohammed; Compact MIMO Antennas and HAP Diversity for High Data Rate Communications, IEEE 64th Semiannual Vehicular Technology Conference, Montreal, Canada, 25-28 September, 2006. T. Hult, A. Mohammed, D. Grace and Z. Yang; Performance of a Multiple HAP System Employing Multiple Polarization, Wireless Personal Multimedia Communications 2006, WPMC06, San Diego, USA, 17-20 September, 2006. T. Hult and A. Mohammed; Combined Polarization and Satellite Diversity For High Data Rate Communications, Antenn 06, Linköping, Sweden, 30 May - 1 June, 2006. T. Hult and A. Mohammed; MIMO Antenna Applications for High Altitude Platforms, Antenn 06, Linköping, Sweden, 30 May - 1 June, 2006. T. Hult and A. Mohammed; MIMO for HAPs: an idea whose time has come, COST 297 - HAPCOS meeting and workshop, Oberpfaffenhofen, Germany, 05-07 April, 2006. T. Hult and A. Mohammed; MIMO Antenna Applications for LEO Satellite Communications , COST 280 - 3rd International Workshop, Prague, Czech Republic, 6-8 June, 2005. A. Mohammed and T.Hult; Performance Evaluation of a MIMO Satellite Diversity System, European Space Agency 10th International Workshop on Signal Processing for Space Communications, SPSC 2008, Rhodes Island, Greece, 6-8 October, 2008. 14 Chapter 4 is published as: T. Hult and A. Mohammed; Assessment of Multipath Propagation for a 2.4 GHz Short-Range Wireless Communication System, IEEE 65th Semiannual Vehicular Technology Conference, Dublin, Ireland, 22-25 April, 2007. T. Hult and A. Mohammed; Multipath Propagation Assessment for a 2.4 GHz Short-Range Wireless Communication System, European Union Conference on Antennas and Propagation, EUCAP2006, Nice, France, 6-9 November, 2006. A. Mohammed and T.Hult; Performance Evaluation of the Bluetooth Link for Indoor Propagation by Measurement Trials and FEMLAB Simulations, Wireless Personal Multimedia Communications 2005, WPMC05, Aalborg, Denmark, 18-22 September, 2005. T. Hult and A. Mohammed; Indoor Propagation Simulations Using FEM for Short-Range Wireless Communication Systems Operating at 2.4 GHz, MMWP05 - Conference on Mathematical Modelling of Wave Phenomena 2005, Växjö, Sweden , 14-19 August, 2005. A. Mohammed and T. Hult; Evaluation of the Bluetooth Link and Antennas Performance for Indoor Office Environments by Measurement Trials and FEMLAB Simulations , IEEE 61st Semiannual Vehicular Technology Conference, Stockholm, Sweden, May 30 - June 1, 2005. Chapter 5 is published as: A. Mohammed and T. Hult; The Effects of MIMO Antenna System Parameters and Carrier Frequency on Active Control Suppression of EM Fields, Radioengineering Journal, Volume 16, Number 1, April, 2007. T. Hult and A. Mohammed; Power Constrained Space-Time Processing for Suppression of Electromagnetic Fields, Invited Paper, First Issue of Journal of Communications Software and Systems (JCOMSS), Volume 1, Number 1, September, 2005. 15 T. Hult and A. Mohammed; Suppression of EM Fields using Active Control Algorithms and MIMO Antenna System, Radioengineering Journal, Vol. 13, Number 3, pp. 22-25, September, 2004. T. Hult and A. Mohammed; Active Signal Processing Algorithms for Controlling Electromagnetic Fields: A Tutorial, Invited Paper, 15th International Congress on Sound and Vibration, ICSV15, Daejeon, Korea, 6-10 July, 2008. T. Hult and A. Mohammed; Performance Evaluation of Adaptive Active Signal Processing Algorithms and MIMO Antenna System for the Reduction of Electromagnetic Field Density, European Union Conference on Antennas and Propagation, EUCAP2007, Edinburgh, UK, 11-16 November, 2007. T. Hult and A. Mohammed; The impact of MIMO Antenna System and Carrier Frequency on Active Control Suppression of Electromagnetic Field, Wireless Networking Symposium 2004, WNCG2004, Austin, USA, 20-22 October, 2004. T. Hult and A. Mohammed, Power Constrained Active Suppression of Electromagnetic Fields Using MIMO Antenna System, 12th International Conference on Software, Telecommunications and Computer Networks, SoftCOM 2004, Co-sponsored by IEEE Communications Society, Split, Croatia, 10-13 October, 2004. T. Hult, A. Mohammed and S. Nordebo; Active Suppression of Electromagnetic Fields using a MIMO Antenna System, 17th International Conference on Applied Electromagnetics and Communications, ICECom 2003, Co-sponsored by IEEE Communications Society, Dubrovnik, Croatia, 1-3 October, 2003. Chapter 6 is published as: T. Hult, D. Grace and A. Mohammed; WCDMA Uplink Interference Assessment from Multiple High Altitude Platform Configurations, EURASIP Journal on Wireless Communications and Networking: HAP Special Issue, Hindawi, Special Issue, April 2008. 16 T. Hult, A. Mohammed and D. Grace; WCDMA Coverage Enhancement from Multiple High Altitude Platforms, COST 297 - HAPCOS meeting and workshop, Nicosia, Cyprus, 7-9 April, 2008. T. Hult, D. Grace and A. Mohammed; WCDMA Capacity and Coverage Enhancement from Multiple High Altitude Platform Configurations, European Union Conference on Antennas and Propagation, EUCAP2007, Edinburgh, UK, 11-16 November, 2007. Chapter 7 is published as: T. Hult and A. Mohammed; Cooperative Beamforming for Wireless Sensor Networks, European Union Conference on Antennas and Propagation, EUCAP2007, Edinburgh, UK, 11-16 November, 2007. 17 Abbrevations and Acronyms 2D 3D 3G AWGN BER BLER BS CAD CDMA CEFM CP DFT DOA DOD DOF EGC ERS FDM FDMA FEM FSL GSM HAP ISM LEO LHCP LMS LOS MIMO MISO MRC NLOS OFDM PD PIFA RHCP Two Dimensional Three Dimensonal Third Generation Additive White Gaussian Noise Bit Error Rate Block Error Rate Base station Computer Aided Design Code Division Multiple Access Combined Empirical Fading Model Cyclic Prefix Discrete Fourier Transform Direction of Arrival Direction of Departure Degrees of Freedom Equal Gain Combining Empirical Roadside (model) Frequency Divison Multiplexing Frequency Division Multiple Access Finite Element Method Free Space Loss Global System for Mobil telecommunication High Altitude Platform Industrial, Scientific and Medical (frequency band) Low Earth Orbit Left Hand Circular Polarized Least Mean Square Line of Sight Multiple-Input Multiple-Output Multiple-Input Single-Output Maximum Ratio Combining No Line of Sight Orthogonal Frequency Division Multiplexing Polarization Domain Printed Inverted-F Antenna Right Hand Circular Polarized 18 RSSI RX SAR SC SD SIMO SISO SINR SNR STP SVD TD TDM TDMA TX UAV UE UMTS WCDMA WSN XPD XPI Received Signal Strength Indicator Receiver Specific Absorption Rate Selection Combining Space Domain Single-Input Multiple-Output Single-Input Single-Output Signal to Interference plus Noise Ratio Signal to Noise Ratio Space Time Polarization Singular Value Decomposition Time Domain Time Division Multiplexing Time Division Multiple Access Transmitter Unmanned Aerial Vehicle User equipment Universal Mobile Telephony System Wideband CDMA Wireless Sensor Networks Cross Polar Discrimination Cross Polar Isolation 19 Symbols and Notations · × ⊗  ∗  R C x x∗ x xi H HT HH H−1 Hij Tr(H) diag {H} ||H||F min x w CN (µ, σ 2 ) E {H} r  E ∇ Jl (x) jl (x) nl (x) hl (x) Scalar product Vector product Kroenecker product (Tensor product) Shur-Hadamard product (Elementwise product) Convolution Circular convolution A set of real valued numbers A set of complex valued numbers Scalar variable The complex conjugate of x Data vector Element i of vector x Data matrix Transpose of matrix H Hermitian transpose, or complex conjugate transpose of matrix H Inverse of matrix H Element in row i, column jof matrix H Trace of matrix: Tr(H) = i Hii Only the diagonal elements of H The Frobenius norm of H: ||H||2F = Tr(HHH ) Minimize x with respect to w Complex valued Gaussian distribution with expected value µ and variance σ 2 E {H} or Statistical expectation of H Field position vector: r = (x, y, z) Field data vector   ∂ ∂ ∂ , ∂y , ∂z Vector gradient operator, ∇ = ∂x Bessel function of the first kind, order l Spherical function of order l: bessel π jl (x) = 2x Jl+0.5 (x) Spherical neuman of order l:  function π nl (x) = (−1)l+1 2x J−l−0.5 (x) Spherical hankel function of order l: hl (x) = jl (x) + ı · nl (x) 20 CHAPTER 1 INTRODUCTION W ireless communication networks are rapidly growing at an incredible rate around the world and a number of emerging technologies are seen to be critical to the improved economics and performance of these networks. Among these technologies, the use of ’space-time processing’ in which time (the natural dimension of digital communication signals) is complemented with the spatial dimension inherent in the use of multiple spatially distributed antennas [10, 11], has appeared as a very promising technology. The use of space-time signal processing can significantly improve average signal power, mitigating fading, and reduce inter-symbol interference and co-channel interference. This can in turn result in significant improvement in energy efficiency, capacity, coverage and quality of wireless systems. Space-time processing can be applied at the transmitter, the receiver or both. Thus, the different antenna configurations used in defining spacetime systems can be classified as follows. Single-input single-output (SISO) is the conventional wireless communication system configuration where the transmitter and receiver utilize a single antenna only. Adding extra antennas makes it possible to exploit the advantages of spatial dimension in the system. A system where multiple antennas are employed at the transmitter only is denoted as multiple-input single-output (MISO) and is said to utilize transmit diversity. Similarly, a system where multiple antennas are employed at the receiver only is denoted as single-input multiple-output (SIMO) and is said to utilize receive diversity. On the other hand, a multiple-input multipleoutput (MIMO) system is enabled by the use of multiple transmit antennas 22 Chapter 1. Introduction and multiple receive antennas in order to take full advantage of the spatial dimension of the propagation channel. MIMO wireless links are important since they improve link reliability through diversity advantage and increase potential data rate through multiplexing gain. Thus, MIMO systems are seen as a critical and promising technology for next generation wireless networks. In this thesis we expand the scope of space-time processing by proposing novel applications in wireless communications. These include enhancing the capacity of satellite and high altitude platform (HAP) communication systems, improving link quality for Bluetooth links in indoor office environments, reduction of the possibly harmful electromagnetic radiation from mobile phones, enhancing the coverage and capacity of integrated multipleHAP 3G systems, and improving the energy efficiency of cooperative wireless sensor networks (WSN). 1.1 Outline of the Thesis and Contributions Chapter 2 In terrestrial wireless communications scenarios, where multipath propagation and signal fading are important issues, the use of adaptive fading mitigation techniques (channel assignment policies, adaptive modulation and coding, equalizers, bit-loading, synchronizers, etc.) can represent fundamental means of achieving a high service availability for critical applications, such as real-time transmissions and broadband communications. In general, the implementation of such adaptive techniques requires knowledge of the time autocorrelation function of the channel. Moreover, since the use of smart antennas is becoming a concrete possibility for both access points at base stations and a wide range of user terminals (personal computers, fixed collective wireless access terminals, laptops, etc.), the spatial autocorrelation function of short-term signal variations has to be modeled as well. As bandwidth is a paramount constraining factor on the number of channels it is possible to multiplex within a limited frequency range, traditionally by using polarization diversity the number of channels can be doubled without the need to increase the bandwidth. Recent research have shown that it is possible to acquire even more channels by using a combination of spatial and polarization diversity [8] in a scattering rich environment. In chapter 2, we propose a novel multiple antenna channel model and associated simulator that is taking into account the spatial, temporal and 1.1. OUTLINE OF THE THESIS AND CONTRIBUTIONS 23 polarization (STP) properties affecting signal transmission in wireless communications [14, 20–23]. In addition, we present the theoretical background, features and properties, analysis and implementation of this STP channel model and simulator. Further, we test the simulator for various propagation conditions. Results show good correspondence between the simulated and theoretical distributions and the adverse effect of depolarization on system performance. The structure of the channel simulator is designed to maintain affordable computational burden, through an efficient time-varying FIR filter bank implementation. Chapter 3 The need for high-speed, high-quality bandwidth efficient mobile communications is continuously growing. In chapter 3, we address the potential gain of using MIMO antenna system in combination with OFDM (orthogonal frequency division multiplexing) in order to enhance the capacity in satellite [7, 14–18] and high altitude platform (HAP) [19–28] communication systems. In particular, we consider the increase in channel capacity that is possible by exploiting the platform (Satellite/HAP) and polarization diversity. In addition, we investigate the effect of the various parameters (e.g. the different compact MIMO antenna array configurations including a novel array denoted as the MIMO-Octahedron, separation angles between platforms, power control, mutual coupling and spatial correlation, cross-polarization discrimination due to weather conditions) on the information theoretic capacity of the total transmission channel of the satellite/HAP system. Simulation results show that the platform diversity system provides superior performance compared to the single platform system, and that the MIMOOctahedron and MIMO-Cube antenna arrays can access twice the number of platforms as the MIMO-Tetrahedron and vector element antenna and thus provide higher capacity. Chapter 4 Over the last decade there has been an explosive growth in the use of wireless mobile communications. Today we find users with mobile phones, wireless PDA’s, MP3 players, and wireless headphones to connect to these devices. In this chapter, we investigate the wave propagation effects of a short-range wireless device, such as the Bluetooth technology. Specifically, we assess the fading phenomenon for Bluetooth link in an indoor office environment by 24 Chapter 1. Introduction simulation of different propagation scenarios [49–53], and use measurement results to confirm our findings. The spatial properties of wireless communication channels are extremely important in determining the performance of wireless systems. Thus, we apply space-time multiple antenna systems employing SIMO antenna diversity system and MIMO antenna system using spatial diversity and spatial multiplexing schemes to the Bluetooth system [51–53] and assess their performance over fading radio channels in non-line of sight propagation environment. Simulation results show a significant diversity and multiplexing gain is achieved by the multiple antenna systems as compared to the SISO antenna system. Chapter 5 Several studies have been conducted on the effects of radiation on the human body. This has been especially important in the case of radiation from hand held mobile phones. The amount of radiation emitted from most mobile phones is very small, but given the close proximity of the phone to the head it might be possible for the radiation to cause harm. In chapter 5 of this thesis we propose a new approach for the reduction of electromagnetic field density at a certain volume in space (e.g. at the human head). The suggested approach involves the use of adaptive active control algorithms and a full space-time processing system setup (i.e. multiple antennas at both the transmitter and receiver side or MIMO), with the objective of reducing the possibly harmful electromagnetic radiation emitted by hand held mobile phones [59–63]. In addition, we also investigate the impact of MIMO antenna parameters, carrier frequency and power constraint on the performance of the system. Simulation results show the possibility of using the adaptive control algorithms and MIMO antenna system to attenuate the electromagnetic field power density. Chapter 6 Third generation mobile systems are gradually being deployed in many developed countries in hotspot areas. However, owing to the amount of new infrastructures required, it will still be some time before 3G is ubiquitous, especially in developing countries. One possible cost effective solution for deployments in these areas is to use High Altitude Platforms (HAPs). 1.1. OUTLINE OF THE THESIS AND CONTRIBUTIONS 25 In this chapter we investigate the performance of utilizing multiple HAPs to provide coverage of a common cell area using a Wideband Code Division Multiple Access (WCDMA) system [110–112]. In particular we study the uplink system performance of the system. The results show that depending on the traffic demand and type of service used, there is a possibility of deploying 3-6 HAPs covering the same cell area. The results also show the effect of cell radius on performance and the position of the multiple HAP base stations which give the worst performance. In addition, we also apply space-time receiver diversity techniques such as single-input multipleoutput (SIMO) or multiple-input multiple-output (MIMO) and compare their performance with that obtained from a single-input single-output (SISO) system. Simulation results show a superior performance is achieved using these diversity techniques and that a practical 4x4 MIMO system provides an optimal system performance. Chapter 7 Wireless Sensor Networks (WSN) have been attracting great attention recently due to the relatively low cost of deployed and usage in many diverse and promising applications, such as biomedical sensor monitoring (e.g., cardiac patient monitoring), habitat monitoring (e.g., animal tracking), weather monitoring (temperature, humidity, etc.), low-performance seismic sensing, environment preservation and natural disaster detection/monitoring (e.g., flooding and fire). These applications have in common the need to send their collected data to some central processing station. If the sensors are located at a faraway distance from a processing node, an inefficient use of bandwidth and transmitter power resources is the result if each wireless sensor is transmitting its measurement data to the base station (processing station). By using a coordinating cluster head, for each cluster of wireless sensor nodes, we can use the combined transmitter power of the node cluster through the use of beamforming or multipath diversity array processing to increase the transmitter-receiver separation and/or to improve the signal-to-noise ratio (SNR) of the communication link. The aim of this chapter is to investigate and assess the beamforming performance of the randomly positioned wireless sensor array and to compare its performance with different forms of diversity array systems (SIMO, MISO and MIMO) [113]. Simulation results show that the diversity systems are superior in performance to both the SISO link and the traditional form of array beamforming. 26 Chapter 1. Introduction CHAPTER 2 A NOVEL SPACE-TIME-POLARIZATION CHANNEL MODEL FOR WIRELESS COMMUNICATIONS O ne of the most common problems encountered in the analysis or design of radio communications systems is the characterization of the propagation channel, since a comprehensive knowledge of the channel features may help the designers toward the selection of suitable solutions to establish reliable communication links. Furthermore, the availability of realistic channel models and effective simulators may be helpful in proving the effectiveness of the selected solution. In terrestrial wireless communications scenarios, where multipath propagation and signal fading are important issues, the use of adaptive fading mitigation techniques (channel assignment policies, adaptive modulation and coding, equalizers, bit-loading, synchronizers, etc.) can represent fundamental means of achieving a high service availability for critical applications, such as real-time transmissions and broadband communications. In general, the implementation of such adaptive techniques requires knowledge of the time autocorrelation function of the channel. Moreover, since the use of smart antennas is becoming a concrete possibility for both access points at base stations and a wide range of user terminals (personal computers, fixed collective wireless access terminals, laptops, etc.), the spatial autocorrelation function of short-term signal variations has to be modeled as well [36]. As bandwidth is a paramount constraining factor on the number of chan- Chapter 2. A Novel Space-Time-Polarization 28 Channel Model for Wireless Communications nels it is possible to multiplex within a limited frequency range, traditionally by using polarization diversity the number of channels can be doubled without the need to increase the bandwidth. Recent research have shown that it is possible to acquire even more channels by using a combination of spatial and polarization diversity [8] especially in a scattering rich environment. However, the independent radio channels are sensitive to depolarizing effects which might cause significant impact on system’s performance. The depolarizing effect can be caused by interference due to weather conditions and from interactions with physical objects that are present in the propagation medium. In light of the above, and the vast interest in Multiple-Input MultipleOutput (MIMO) systems, multicarrier transmission employing Orthogonal Frequency Division Multiplexing (OFDM) and compact MIMO antenna array configurations, new and improved channel models are necessary to evaluate the parameters and performance of these system. Thus, in this chapter we propose a novel multiple antenna channel model and associated simulator that take into account the spatial, temporal and polarization (STP) properties affecting signal transmission in wireless communications. In addition, we provide the theoretical background, features and properties, analysis and implementation of this STP channel model and simulator. Further, we test the simulator for various propagation conditions. The proposed channel model and simulator are designed for link level simulations and is an extension of the model presented in [36], where only the spatial and temporal properties of the signals were implemented. The proposed channel simulator provides a powerful tool for evaluating the performance of current and future communication systems. However, it is designed to maintain an affordable computational burden with the use efficient time-varying FIR filter bank implementation. The organization of this chapter is as follows. Section 2.1 presents the theoretical background, features and properties, analysis and implementation of the proposed space-time-polarization (STP) channel model. Section 2.2 present the simulation results and provide evaluations and performance comparisons of the parameters for different propagation scenarios. Finally, section 2.3 concludes this chapter. 2.1 Space-Time-Polarization Channel Model In this section we present the theoretical background, features and properties, analysis and implementation of the proposed space-time-polarization (STP) 2.1. SPACE-TIME-POLARIZATION CHANNEL MODEL 29 channel model and the associated simulator. Each object in the propagation channel is modeled as a cluster of micro-scatterers [36], see figure 2.1, in the local area (within a few hundred wavelengths) centered about the center position of the cluster. This cluster is denoted as a macro-scatterer. Furthermore, both the transmitter and the receiver can respectively be positioned inside a local area surrounded by micro-scatterers. The clusters are modeled in order to calculate the angle spreading effect and depolarization due to reflection, diffraction, and scattering off objects in the non line-ofsight (NLOS) propagation environment plus the scintillation phenomena and depolarization effects due to precipitation and Faraday rotation phenomena in the direct line-of-sight (LOS) path as well [14, 21–23]. With the presence of different polarizations, the attenuations, phase shifts and depolarizations generated by the multipath cluster interaction can differ for different incident polarization states and will therefore also generate a cross-polarization effect. 2.1.1 Space-Polarization Channel Model The signals carried by the different sub-channels of a multiple-input multipleoutput (MIMO) communications system are written in a vector format as T  i(t)  i(1) (t), i(2) (t), · · · , i(Np )(t) , (2.1) where i(p) (t) is the information signal transmitted with the pth sub-channel. The transmitting antenna is assumed to be a linear transformation of the input signal i(t) into the independent radio sub-channels s(t), according to s(t)  MTtx i(t), (2.2) At the receiver we have a similar transformation from the signals in the independent radio sub-channels srx (t) into the output signal r(t) of the system, i.e. the vector of the elementary signals received in each sub-channel, T  r̂(t)  r̂(1) (t), r̂(2) (t), · · · , r̂(Np )(t) = Mrx srx (t), (2.3) where s(t) and srx (t) are vectors containing the independent spatial-polarization sub-channels that are active for a specific antenna type and they are related through (2.4) srx (t) = Hch ∗ s(t), Chapter 2. A Novel Space-Time-Polarization 30 Channel Model for Wireless Communications TX antenna local area Local area Micro-scatterer Doppler angle LOS path Angle of Departure l-th Macro scatterer l-th LOS Cluster Depolarization Depolarization l-th Cluster Angle of Arrival Angle spread Local area Micro-scatterer RX antenna local area Figure 2.1: The cluster geometry for the space-time-polarization simulator. 2.1. SPACE-TIME-POLARIZATION CHANNEL MODEL 31 where the symbol ∗ indicates matrix convolution, as defined in [36]. The channel Hch , from the transmitter sub-channel vector s(t) to the receiver sub-channel vector srx (t), is the simulated propagation channel. Thus, the sub-channel signal vector r̂(t) at the receiver can be rewritten using equations 2.2, 2.3 and 2.4 as a linear combination of all the transmitted sub-channel, each of which is subjected to the effects of the propagation environment r̂(t) = Mrx Hch ∗ MTtx i(t). (2.5) The coefficients of the linear combination represent the effect of the fading, cross-correlation and depolarization induced by the channel environment. Elementary channel matrix In general, it is possible to assume that each sub-channel is transmitted by an antenna array that uses a specific spatial processor (transmitter beamformer) for each specific sub-channel. The pth transmitter beamforming weight vector is then denoted as v(p) . The signals propagating through the wireless channel are affected by several factors (e.g. spatial and temporal fast fading, shadowing, etc.), in which the short-term fast effects are considered in [36]. In particular, the signals are affected by reflection, diffraction and scattering phenomena, both at macroscopic and microscopic (scattering) scale that generates attenuations, phase shifts and time delays. It also causes the signals to arrive at the receiver from different Direction of Arrivals (DOA’s) of the direct LOS path. This is characterized by a certain angular spread of the signals. There is also the possibility of mobility at both transmitter and receiver side, which contributes to the scattering phenomenon and give rise to temporal fading processes. However, in the presence of different polarizations the attenuations and phase shifts generated by the microscopic interactions with the scattering structures may differ for different polarizations and could generate cross-polar effects. From equation 2.5 the elementary signal received in the pth sub-channel can be written as p r̂ (t) = w (p)H arx (θ) Np  γqp atx (ξ)v(q) h(ζ; t) ∗ i(q) (ζ), (2.6) q=1 where w(p) is the receiver beamforming weight vector used for the pth subchannel, atx (ξ) and arx (θ) are the transmitter and receiver array steering Chapter 2. A Novel Space-Time-Polarization 32 Channel Model for Wireless Communications vectors respectively. ξ and θ are the Direction of Departure (DOD) and Direction of Arrival (DoA) expressed with respect to the transmitter and receiver reference frame. h(ζ; t) is the time-domain elementary path impulse response defined in [36], ∗ is the convolution operator, and γqp is the real coefficient cross polarization discrimination (XPD), representing the fraction of the q th polarization being scattered into the pth part E E⊥→ E = , E⊥← γqp = (2.7) γpq (2.8) where E is the amount of the signal that is still in the original transmitted polarization state and E⊥→ is the the fraction of the transmitted signal that has been rotated into the opposite orthogonal polarization state. Assuming p ⊥ and q . Furthermore,  (2.9) aTtx (ξ)v(p) = MTtx (q,q) w(p)H arx (θ) = [Mrx ](p,p) , (2.10) since from equations 2.2 and 2.3 it is possible to set the relationships Mtx  Dv ⊗ atx (ξ) Mrx  Dw ⊗ arx (θ), where ⎡ 0 0 .. . v(2) 0 ··· ⎢ ⎢ Dv  ⎢ ⎢ ⎣ v(1) ··· .. . (2.11) (2.12) ⎤ 0 .. ⎥ . ⎥ ⎥ ∈ CN Np ,Np . ⎥ ⎦ (2.13) v(Np ) Dw ∈ CM Np ,Np is defined in a similar way and ⊗ indicates the Kronecker product. The expression in equation 2.6 can then be rewritten in matrix notation as   (2.14) r̂p (t) = w(p)H arx (θ) γ (p)T ⊗ aTtx (ξ) Dv h(ζ; t) ∗ i(ζ), where  γ (p)  γ11 , γ21 , · · · , γNp ,1 T . (2.15) 2.1. SPACE-TIME-POLARIZATION CHANNEL MODEL 33 The vector of the received elementary sub-channels, i.e. the vector of the elementary signals received in each sub-channel, can now be expressed as T  (2.16) r̂(t)  r̂(1) (t), r̂(2) (t), · · · , r̂(Np ) (t) =   ⎤ ⎡ w(1)H arx (θ) γ (1)T ⊗ aTtx (ξ) Dv h(ζ; t) ∗ i(ζ) ⎥ ⎢ .. =⎣ (2.17) ⎦= .   (Np )H (Np )T T arx (θ) γ ⊗ atx (ξ) Dv h(ζ; t) ∗ i(ζ) w   H T T (2.18) = Dw Γ ⊗ arx (θ)atx (ξ) Dv h(ζ; t) ∗ i(ζ), where   Γ  γ (1) , γ (2) , · · · , γ (Np ) = ⎡ ⎤ γ11 γ12 · · · γ1Np ⎢ .. ⎥ ⎢ γ21 γ22 . ⎥ ⎢ ⎥ ∈ RNp Np =⎢ . ⎥ . .. ⎣ .. ⎦ γNp 1 · · · γNp Np (2.19) (2.20) is the cross-polarization matrix. Thus, it is possible to define the multi antenna space-polarization elementary path channel matrix as ˆ H(ζ, t)  ΓT ⊗ arx (θ)aTtx (ξ)h(ζ, t) ∈ CM Np Np . (2.21) This is also depicted as a block diagram in figure 2.2, where we can identify the elementary-path channel matrix Ĥ(ζ, t) = arx (θ)aTtx (ξ)h(ζ, t) obtained in [36]. Thus, ˆ H(ζ, t) = ΓT ⊗ Ĥ(ζ, t), (2.22) and the received elementary sub-channel vector becomes ˆ r̂(t) = DH w H(ζ, t) ∗ Dv i(ζ), (2.23) ˆ T which allows the equivalence, DH w H(ζ, t)Dv ≡ Mrx Hch Mtx , as derived from equation 2.5. Global Multi Space-Polarization Channel Matrix Following the analogy developed in [36], it is possible to identify the th cluster multi antenna space-polarization channel matrix for each cluster of Chapter 2. A Novel Space-Time-Polarization 34 Channel Model for Wireless Communications Figure 2.2: The block diagram of the complete multiple antenna STP simulator: (top figure) the signal from each transmitting antenna element is filtered by a separate space-time-polarization FIR filter, and (bottom figure) FIR filter block for each cluster. 2.1. SPACE-TIME-POLARIZATION CHANNEL MODEL 35 microscopic scattering elements in the physical channel. Thus, indicating with D(χ) the multi-dimensional domain of the vector of the independent T channel variables χ  [ξ, θ, ψtx , ψrx ] with its nominal value χ for each cluster  = 0, 1, · · · , LS . The th cluster channel matrix can then be computed as   ˆ H (ζ, t)  H(ζ, t)dχ = ΓT ⊗ arx (θ)aTtx (ξ)h(ζ, t)dχ. (2.24) D(χ ) D(χ ) The global multi space-polarization channel matrix can now be written as, H(ζ, t)  LS  H (ζ, t). (2.25) =0 where H(ζ, t) is the total multi antenna space-time-polarization channel simulator model. We can now write the received signal vector r̂(t) using equations 2.2, 2.3 and 2.4, where we define Hch  H(ζ, t), as a linear combination of all the transmitted sub-channels: r̂(t) = Mrx Hch ∗ MTtx i(t). (2.26) The coefficients of the linear combination represent the effect of the spatiotemporal fading, cross-correlation and depolarization induced by the channel environment. 2.1.2 Statistical properties of the global channel matrix From [36] we find that the characterization of the global channel matrix is a stochastic process in order to take into account the statistical variations of the physical effects of the micro-scatterers on the propagating signal. Most of the assumptions and properties stated in [36] for the spatiotemporal channel matrices H (ζ, t) are still valid for the multiple space-timepolarization channel matrices H (ζ, t) and will briefly be analyzed in this chapter. A few extra assumptions and properties are also discussed, related to the specific structure of the cross-polarization matrices. Assumption 1. Clusters are statistically independent to one another and therefore there is no correlation between different multiple antenna spacepolarization cluster matrices H (ζ, t) and Hm (ζ, t),  = m, nor is there any correlation between their constituent multiple antenna space-polarization elementary path sub matrices. Chapter 2. A Novel Space-Time-Polarization 36 Channel Model for Wireless Communications Assumption 2. The random part of the channels elementary path sub matrices is characterized by: 1. the amplitude attenuation αSC and phase shift ejϕSC related to the micro-scatterers, and behave in the same way for any polarization state. 2. the cross-polarization factors, γqp, , which represent the amount of the q th polarization state that is rotated into the pth polarization state by the th cluster. The random variables γqp, , αSC and ϕSC are assumed to be statistically independent and the random phase ϕSC is uniformly distributed in [0, 2π). Furthermore, the random variables associated with different clusters are also assumed to be independent. As a consequence of the last assumption, the following properties can be inferred. Property 1. The cross-polarization matrix Γ consists of random variables, whose probability distribution depends on the physical nature of the cluster. Proof. Follows directly from Assumption 2. Property 2. The multiple antenna space-time-polarization th cluster channel matrix can now be written as  ˆ H (ζ, t) = Γ ⊗ H(ζ, t)dχ. (2.27) D(χ ) Proof. Directly inferred from Property 1. The structure of the th cross-polarization matrix Γ is described in equation 2.19. Assumption 3. The Doppler effect angles ψT X , ψRX are assumed to be independent of each other and of any other stochastic variable in the channel model. Assumption 4. The extra time delay τ is a constant value for all the elementary paths of a particular cluster. Property 3. Each multiple antenna polarization cluster matrix H (ζ, t) is a matrix of zero-mean circular complex Gaussian random variables, conditioned by the cross-polarization factor. 2.1. SPACE-TIME-POLARIZATION CHANNEL MODEL 37 Proof. If we identify the constituent blocks of the multiple antenna polarization th cluster channel matrix, ⎡ [H ]11 (ζ, t) ⎢ ⎢ [H ]21 (ζ, t) H (ζ, t) = ⎢ ⎢ .. ⎣ . [H ]12 (ζ, t) ··· [H ]22 (ζ, t) .. ··· [H ]Nq 1 (ζ, t) . ⎤ [H ]1N p (ζ, t) ⎥ .. ⎥ . ⎥, ⎥ ⎦ (2.28) [H ]Nq Np (ζ, t) where [H ]qp (ζ, t)  γqp H (ζ, t). (2.29) Conditioned on γqp , the distribution of the matrix entries is circularly complex Gaussian with zero mean. Through applying the Central Limit Theorem to expressions in equation 2.24 and 2.25, we can infer that each matrix entry is a circularly complex Gaussian random variable, since they are defined as a superposition of an infinite number of stochastic contributions. Furthermore, because of the uniformly distributed random phase ϕSC , the statistical mean value of the cluster matrix is given by    ΓT ⊗ arx (θ)aTtx (ξ)E {h(ζ, t)} dχ = (2.30) E H (ζ, t) = D(χ )  vT X vRX = αF S (τ )e−jω0 τ δ(ξ − τ ) · e−jω0 c t cos(ψT X ) e−jω0 c t cos(ψT X ) · D(χ ) ·Γ ⊗ T arx (θ)aTtx (ξ)E  jϕSC e  (2.31) dχ = 0, (2.32) where E {·} denotes statistical expectation. Now we calculate the mutual correlation matrix of the entries of the multiple antenna polarization th cluster matrix. To do this, we redefine the vector h (ζ, t) as (2.33) h (ζ, t)   T    T vec [H ]11 (ζ, t) , vec [H ]21 (ζ, t) , · · · ,       vecT [H ]Nq 1 (ζ, t) , vecT [H ]12 (ζ, t) , · · · , vecT [H ]Nq Np (ζ, t) . Chapter 2. A Novel Space-Time-Polarization 38 Channel Model for Wireless Communications It is now possible to reformulate this by inspecting the above expression and rewriting it as h (ζ, t) = vec {Γ } ⊗ vec {H (ζ, t)} , (2.34) so that it is easy to see that the following properties are valid. Property 4. Vectors h (ζ, t), hm (ζ, t),  = m, are statistically independent. Proof. Directly derived from Assumption 2. Property 5. Vectors h (ζ, t),  = 0, 1, . . . , LS are wide-sense stationary (WSS) random processes with respect to the time variable t. Proof. The vectors have zero mean, as shown in equation 2.30. Furthermore, their stationarity with respect to the time variable t can be proved as follows.   (2.35) R (ζ,t1 , t2 )  E h (ζ, t1 )hH  (ζ, t2 ) =   H =E (vec {Γ } ⊗ vec {H (ζ, t)})(vec {Γ } ⊗ vec {H (ζ, t)}) =     H H =E vec {Γ } vec {Γ } ⊗ E vec {H (ζ, t)} vec {H (ζ, t)} , where we used the fact that the cross-polarization factors are statistically independent from any other random variable, as stated in Assumption 2. Thus, by defining the Polarization-Domain (PD) th cluster autocorrelation matrix as   2 2 (2.36) RP D,  E vec {Γ } vecH {Γ } ∈ RNq ,Np , and using known results [36] about the Time and Space domain autocorrelation matrices, we can now write R (ζ, t1 , t2 ) = RP D, ⊗ RT D, (ζ, t1 − t2 )RSD, = R (ζ, ∆t), (2.37) which demonstrates wide-sense stationarity with respect to time. So far, we have presented the structure of the multiple antenna spacepolarization cluster channel matrix and its autocorrelation. We will now define the structure of the simulator by implementing the channel model. The separability of the polarization domain and the space and time domains, as concluded from equation 2.37, preserves the validity of the spatial and temporal characterizations, while it also allows the characterization of the cross-polarization component as shown in equation 2.19. 39 2.1. SPACE-TIME-POLARIZATION CHANNEL MODEL 2.1.3 Numerical Implementation The structure of the multiple antenna space-polarization simulator which includes cross-polarization effects is that each transmitting antenna have Np space-polarization sub-channels (i.e., Np signals) and the FIR filter structure of [36], creates the spatio-temporal fading effects. In figure 2.2 we show the simulator for which Np = 2 different space-polarization sub-channels are (p) presented for simplicity. Let sn [k] be the signal sample taken at the time instant t = kTc , of the signal transmitted by the nth transmitting antenna using the pth space-polarization sub-channel, according to ∗(p) (p) (kTc ), s(p) n [k]  vn i (2.38) (p) where Tc is the sampling time used in the simulation and vn is the nth element of the transmitting beamforming weight vector used for the pth space(p) polarization sub-channel. Then, let xm,n [k] be the amount of the k th sample generated by the contribution of the nth transmitting antenna of the signal received at the mth receiving antenna through the pth space-polarization subchannel. It is then the faded and cross-polarized pth signal along the n−to−m path of the channel, represented in figure 2.2. The effect of the multiple antenna space-polarization channel on the n − to − m path, apart from the additive noise, can now be written as ⎡ ⎤ Np LS   ⎣bn,m, [k] ⎦ γqp, s(q) δ0 = 0, (2.39) x(p) m,n [k] = n [k − δ ] , =0 q=1 where bn,m, [k] is the th filter tap at the time instant k and δ is the associated time delay. In the above formulation it is worth to recognize that the fading filter coefficients bn,m, [k] are multiplied every time by the cross-polarization factors γqp, in matrix Γ . The complete multiple antenna space-time-polarization simulator generates its filtering coefficients, including the cross-polarization factors, in the following procedure. Property 6. In order to guarantee that the coefficients of the FIR filtering structure in figure 2.2 have the autocorrelation function expressed in equation 2.37, they are implemented as follows. 1.  = 0. 2. begin loop Chapter 2. A Novel Space-Time-Polarization 40 Channel Model for Wireless Communications 3. Generate (N × M ) independent zero-mean complex white Gaussian processes G ∈ CN M,KS , where KS is the number of discrete samples to be simulated. 4. Correlate the processes G in the temporal and spatial domain • Design a time correlation shaping filter with transfer function T (z), such that the time autocorrelation of the output process is RT D, (ξ, δt). • Then, filter each row of G with T (z), obtaining the matrix of timefiltered processes GT,  . • Compute the eigenvector decomposition of the spatial autocorrelation matrix (2.40) RSD, = USD, ΛSD, UH SD, .  • Generate the matrix S  USD, ΛSD, ∈ CN M,N M . • Compute the matrix B  S GT, ∈ CN M,Ks , containing all the fading coefficients for the th cluster from each transmitting antenna element to each receiving antenna element, and for the time index, k = 0, 1, . . . , KS − 1. to obtain the fading matrix B ∈ CN M,KS . 5. Generate Np2 independent zero-mean real white Gaussian stochastic 2 variables c ∈ RNp . 6. Compute the eigenvector decomposition of the polarization domain autocorrelation matrix RP D, = UP D, ΛP D, UH P D, . 7. Generate the matrix XP D,  UP D, (2.41)  2 2 ΛP D, ∈ CNp Np . 8. Assign the proper correlation in the polarization domain to the vector c , as (2.42) γ̂  XP D, c . 9. Assemble the estimated th cross-polarization matrix Γ̂ from γ̂ , using   (2.43) γ̂ = vec Γ̂ . 2.2. SIMULATION RESULTS 41 10.  =  + 1. 11. repeat loop until  = LS . Proof. If we consider the filtering coefficient used at the time instant k, and th tap, the space-time domain coefficients are written in the k th column of the matrix B , i.e. bk,  [B ]:,k . We can see that the coefficients of the multiple antenna space-polarization simulator in figure 2.2 can be written as Γ̃ ⊗bk, , or in a more convenient vector format as γ̃ ⊗bk, . Thus, the mutual correlation function of these coefficient vectors can be computed as     E (γ̃ ⊗ bk, )(γ̃ ⊗ bk, )H = E γ̃ γ̃H ⊗ bk, bH k, =  H    XP D, ⊗ E bk, bH = XP D, E c cH  k, = = UP D, ΛP D, UH P D, ⊗ RT D, [k − t]RSD, = = RP D, ⊗ RT D, [k − t]RSD, , (2.44)  H = INp2 , from property 6 statement 5 and where we used the fact that E cc   H in equation 2.41, and E bk, bk, = RT D [0]RSD . 2.2 Simulation Results In this chapter we present the simulation results showing some of the features and capabilities offered by the proposed novel multiple antenna STP channel simulator. In addition, we test the simulator performance under different conditions, by considering both LOS and NLOS propagation scenarios. A communication link operating at 2.4 GHz carrier frequency and Tc = 10µs sampling time is simulated, where both the transmitter and receiver utilize a twelve-element Cube shaped linear 3D array (MIMO-Cube antenna) [9]. The receiver is assumed to be moving, while the transmitter is stationary. The long-term fading power values are normalized so that the total received power in non-LOS (NLOS) propagation is 0 dBW, while, in the case of LOS propagation, a Rice factor (K) of 10 dB is assumed. Only one reflection due to a macro-scatterer is simulated, together with the direct path, with relative delay of 600 ns. In the LOS propagation scenario without cross-polarization, the normalized distribution of the channel coefficients is shown in figure 2.3, where a good correspondence is achieved between the simulated LOS distribution, shown by solid blue line, and the theoretical Rice distribution, shown by the solid red Chapter 2. A Novel Space-Time-Polarization 42 Channel Model for Wireless Communications 0.45 Simulated LOS K = 10 dB. Theoretical Rice distrib., K = 10 dB. 0.4 0.35 0.3 0.25 0.2 0.15 0.1 0.05 0 0 5 10 Normalized envelope r 15 20 Figure 2.3: The envelope distribution of the simulated received signals in a LOS propagation environment with a Rice factor K = 10 dB, compared with the theoretical Rice distribution. 43 2.2. SIMULATION RESULTS 0.4 Simulated LOS original K = 10, XPD = 10dB Theoretical Rice distrib. K = 2. 0.35 0.3 0.25 0.2 0.15 0.1 0.05 0 0 5 10 15 20 Normalized envelope r 25 30 35 Figure 2.4: The envelope distribution of the simulated received signals in a LOS propagation environment, with an original Rice factor K = 10 dB and an XPD of 10 dB, compared with the theoretical Rice distribution. line. Due to the high Rice factor (K = 10 dB), most of the received signal power is concentrated along the direct LOS path. Figure 2.4 show the probability distribution of the same signal as in figure 2.3, but with a cross-polarization of XPD = 10 dB. It is evident from comparing these figures that the depolarization between the two polarization states is transforming the original signal with Rice distribution and Rice factor K = 10 dB into a Rice distribution of K = 2 dB. The depolarization effect can also be seen from the time series of the fading coefficients presented in figure 2.5 where deep fading dips are clearly observed for the case of XPD = 10 dB, and thereby adversely affecting the performance of the communications channel. From this observation, we can also conclude that the XPD has similar effect as ’blocking objects’ in the channel propagation environment. Figure 2.6 shows the normalized distribution of the fading coefficients envelope magnitude in a NLOS environment. As expected, it follows a Chapter 2. A Novel Space-Time-Polarization 44 Channel Model for Wireless Communications 16 14 Normalized envelope r [dB] 12 10 8 6 4 2 0 ï2 with no depolarization XPD = 10 dB 0 0.5 1 1.5 Time t [s] 2 2.5 3 ï3 x 10 Figure 2.5: The time series of the received signal in the LOS environment with Rice factor K =10 dB: (blue) without XPD and (red) with XPD of 10 dB. 45 2.2. SIMULATION RESULTS 0.4 Simulated NLOS. Theoretical Rayleigh distribution. 0.35 0.3 0.25 0.2 0.15 0.1 0.05 0 0 1 2 3 Normalized envelope r 4 5 Figure 2.6: The envelope distribution of the simulated received signals in a NLOS scattering environment compared with a theoretical Rayleigh distribution. Chapter 2. A Novel Space-Time-Polarization 46 Channel Model for Wireless Communications 0.4 Simulated NLOS XPD = 10 dB. Theoretical Rayleigh distribution. 0.35 0.3 0.25 0.2 0.15 0.1 0.05 0 0 1 2 3 Normalized envelope r 4 5 Figure 2.7: The envelope distribution of the simulated received signals in a NLOS propagation environment, with an XPD of 10 dB, compared with the theoretical Rayleigh distribution. Rayleigh distribution. The simulated distribution is shown by the blue solid line, while the theoretical Rayleigh distribution analytically obtained from the input parameters of the simulator is shown by the red solid line. A good agreement between the simulated and theoretical data is observed. Figure 2.7 shows the probability distribution of the same signal as in figure 2.6, but with a cross-polarization of XPD = 10 dB. By comparing these figures we can see that there is no difference in the distributions. In addition, by observing the time series of the signal no effect on the fading dips was noticed in this case, however an increase in attenuation of the total signal was observed. 2.3. CONCLUSIONS 2.3 47 Conclusions In this chapter we presented a novel multiple antenna channel model and associated simulator which takes into account the spatial, temporal and polarization (STP) properties affecting signal transmission in wireless communications. In addition, we have presented the theoretical background, features and properties, analysis and implementation of the proposed STP channel model and simulator. Further, we tested the simulator for various propagation conditions, and the simulation results have shown good agreement with the theoretical distributions. Finally, we investigated the impact of depolarization on the probability distributions of the simulated signals and their adverse effect on performance. The proposed channel model and simulator are designed for link level simulations for various communication links where both the transmitter and the receiver are equipped with with an array of antennas. In the next chapter we will employ this simulator for investigating the performance of satellite [7, 14–18] and high altitude platform [19–28] communication links. Chapter 2. A Novel Space-Time-Polarization 48 Channel Model for Wireless Communications CHAPTER 3 SPACE-TIME-POLARIZATION PROCESSING FOR CAPACITY ENHANCEMENT IN HAP/SATELLITE COMMUNICATION SYSTEMS I t has been widely recognized that the capacity in wireless communication systems can be greatly increased by exploiting environments with rich scattering such as urban areas or indoors. Classically, it is well understood that the electromagnetic polarization of plane waves possesses two independent channels, or polarization states [2, 3]. However, it has been shown that the existence of a scattering rich environment can increase the number of combined spatial-polarization channel states and thus effectively increase the channel capacity of the system [6–12]. Independent spatial-polarization or frequency channels can be accessed by means of multiple antennas and the use of orthogonal frequency division multiplexing (OFDM) at both the transmitter and the receiver, thus the technique is referred to as multiple-input multiple-output orthogonal frequency division multiplexing (MIMO-OFDM) communication system. In this chapter we consider the MIMO-OFDM technique as a means of achieving independent channels. In essence, the MIMO technique achieves orthogonality over space and polarization domains by employing the Singular Value Decomposition (SVD), and the OFDM technique achieves orthogonality over the frequency domain by employing the Discrete Fourier Transform (DFT) in conjunction with a Cyclic Prefix Chapter 3. Space-Time-Polarization Processing for Capacity 50 Enhancement in HAP/Satellite communication systems (CP) inserted to reduce the intersymbol interference (ISI) without losing the orthogonality among the sub-carriers and therefore, equalization at the receiver is relatively simple. The aim is to study the theoretical potential of exploiting the spatialpolarization diversity provided by compact MIMO antenna array configurations (e.g., the vector element [7, 8], the MIMO-Cube [9], the MIMOTetrahedron [13] and the novel MIMO-Octahedron array antennas) to achieve higher capacity in communication systems. For example, an application that utilize the spatial-polarization channels is a high data rate transmission system employing multiple satellites in designated orbits [14–18] or high altitude platforms in the stratosphere [19–28]. Satellite communication systems today operate in a variety of frequency bands, ranging from 100 MHz to 100 GHz. Low-Earth-Orbit (LEO) satellite systems like ORBCOMM, E-SAT and LEO ONE [29] that operate in the frequency range 100 to 400 MHz and with a bandwidth of a few MHz are examples of low bit-rate systems that could benefit from the proposed MIMOOFDM multiple platform diversity technique. High Altitude Platforms (HAPs), on the other hand, are quasi-stationary aerial platforms consisting of either unmanned airships or planes that will operate in the stratosphere, 17-22 km above the ground. This emerging technology preserve many of the advantages of both satellite and terrestrial systems [30–34] and has presently started to attract considerable attention in Europe. Using narrow bandwidth repeaters on HAPs for high speed data traffic have several advantages compared to using satellites, especially when operating in a local geographical area. One of the main advantages is that the received signal from the HAP is much stronger than a received signal of equal transmitted power from a satellite. This allows for a much lower transmitter power which would decrease the size and weight of the repeater equipment carried by the HAP. In addition HAPs offer much easier deployment than satellites and so high-speed connection can be made on demand for a specific geographical area. The proposed platform diversity system consists of virtual MIMO spatial channels (created by a multiple relaying platform diversity) in conjunction with the polarization and antenna pattern diversity (formed via special compact MIMO antenna arrays). Various compact MIMO antenna array configurations are investigated and their performance, in term of capacity, is analysed. In addition, since these special compact MIMO antenna array configurations depend on the array elements being positioned very closely together, the effect of mutual coupling and spatial correlation will also be 3.1. PLATFORM DIVERSITY 51 analysed and taken into account when performing the simulation for this combined diversity system. We also investigate the influence of the separation angle between the multiple platforms on system performance, and determine the optimal separation angles that maximize the total capacity of the system for the various compact MIMO antennas. In the proposed scheme, we aim to preserve the orthogonality of polarization states in order to achieve the optimal theoretic capacity performance of the system. However, the independent radio channels utilized in this system are sensitive to depolarizing effects which might cause significant impact on system’s performance. The depolarizing effect can be caused by interference at different layers of the atmosphere. The signals suffer mainly tropospheric effects due to rain and ice particles and ionospheric effects due to the Faraday rotation phenomena. To reinforce the analysis, we present a novel multi-channel simulator that produces realistic time-series of the fading process affecting signal transmission in the proposed platform diversity system. The proposed simulator takes into account the temporal, spatial and polarization properties affecting these processes. Further, we will determine the impact on the total capacity of the proposed application that utilizes the spatial-polarization channels for high data rate transmission system using a multiple platform spatio-polarized compact MIMO antennas system. The organization of this chapter is as follows. Section 3.1 presents the platform diversity system and the utilized channel models. Section 3.2 investigates the use of MIMO-OFDM and power control to further enhance the system capacity. Section 3.3 present the structures of the various compact MIMO antenna arrays. The depolarization analysis and definition of the cross-polar discrimination and cross-polar isolation parameters and their effect on system performance is presented in section 3.4. Section 3.5 present the simulation results and provide evaluations and performance comparisons of the different parameters. Finally, section 3.6 concludes the chapter. 3.1 Platform Diversity In this chapter we propose an application for high data rate transmissions using a system of multiple LEO-satellites [14–18] or High Altitude Platforms (HAP) [19–28]. This system consists of virtually created MIMO channels in the space domain using platform diversity in conjunction with 3D polarization [4, 5] and radiation pattern diversity of a special MIMO antenna arrangement [7, 8] and also through using the OFDM technique. The investigations are Chapter 3. Space-Time-Polarization Processing for Capacity 52 Enhancement in HAP/Satellite communication systems Scenario 1 2 3 4 5 6 7 8 Table 3.1: Platform Scenarios. Platform Number of Platforms Type of Channel Model Satellite 3 FSL Satellite 6 FSL Satellite 3 Multiple STP Satellite 6 Multiple STP HAP 3 FSL HAP 6 FSL HAP 3 Multiple STP HAP 6 Multiple STP HAP b HAP a HAP c 20 km Tx Rx Figure 3.1: The MIMO-HAP diversity system with three HAPs (scenario 5) and the channel paths from the transmitter to the receiver. divided into eight scenarios, see Table 3.1. The number of platforms used in the different scenarios is dependent on the number of channels created by the employed antenna arrays. The antenna arrays investigated in this chapter divide the scenarios into two groups which utilize a platform diversity consisting of three or six relaying platforms. Figure 3.1 and figure 3.2 show the diversity setup for scenarios 5 and 6, respectively. In these two scenarios we assume that the HAPs are located along a fixed line with the HAPs uniformly distributed and separated by the angles θ. A similar setup is produced for the LEO-satellite platforms in scenarios 1 and 2, where three or six satellites are used. These satellites are assumed to 53 3.1. PLATFORM DIVERSITY 20 km Tx Rx Figure 3.2: The MIMO-HAP diversity system with six HAPs (scenario 6) and the channel paths from the transmitter to the receiver. be uniformly located along a fixed orbit with a constant angle of separation. These two scenarios are shown in figure 3.3 and 3.4. In the scenarios (1, 2, 5 and 6) the wave propagation channel Hch from the N transmitter antenna array elements to the M receiver antenna array elements is modeled as a free space loss (FSL) model [12], and is defined as a transformation containing the space dependent decaying values of the signal being transmitted c , (3.1) Hmn (r, f ) = 4πf |rm − rn | where |rm − rn | is the distance along the path between transmitter array element m and receiver array element n. In this propagation channel there are no atmospheric or multipath interference and the noise in the system is modeled as uncorrelated Gaussian noise. For scenarios 3, 4, 7 and 8, a novel space-time-polarization (STP) multi channel simulator model, proposed in chapter 2, is utilized. In these scenarios, a signal transmitted through a propagation channel with physical objects that generates multipath components of the transmitted signal, each with its own attenuation, polarization, correlation, phase shift, delay and direction of propagation. Depending on the material of the objects in the channel, a frequency dependent stochastic scattering effects can also affect the received signal. Each object in the propagation channel is modeled as a cluster of microscatterers [36], see Figure 2.1 in chapter 2, in the local area (within a few Chapter 3. Space-Time-Polarization Processing for Capacity 54 Enhancement in HAP/Satellite communication systems Rx Tx qs qs Figure 3.3: The MIMO-Satellite diversity system with three satellites (scenario 1) and the channel paths from the transmitter to the receiver. 55 3.1. PLATFORM DIVERSITY Rx Tx qs Figure 3.4: The MIMO-Satellite diversity system with six satellites (scenario 2) and the channel paths from the transmitter to the receiver. Chapter 3. Space-Time-Polarization Processing for Capacity 56 Enhancement in HAP/Satellite communication systems hundred wavelengths) centered about the center position of the cluster. This cluster is denoted as a macro-scatterer. Furthermore, both the transmitter and the receiver can respectively be positioned inside a local area surrounded by micro-scatterers. In order to model the atmospheric angle spreading effect due to scintillation phenomena and depolarization effects due to precipitation and Faraday rotation phenomena, clusters are added in the direct line-of-sight (LOS) path as well [14, 21–23]. With the presence of different polarizations, attenuations, phase shifts and polarizations generated by the multipath cluster interaction with the signal can differ for different incident polarization states and will therefore also generate a cross-polarization effect. 3.1.1 Space-Polarization Channel Model The signals carried by the different space-polarization modes (or sub-channels) are written in a vector format as T  (3.2) i(t)  i(1) (t), i(2) (t), · · · , i(Np )(t) , where i(p) (t) is the information signal transmitted with the pth mode. The transmitting antenna is assumed to be a linear transformation of the input signal i(t) into the independent radio channels s(t), according to s(t)  MTtx i(t), (3.3) At the receiver we have a similar transformation from the signals in the independent radio sub-channels srx (t) into the output signal r(t) of the system, i.e. the vector of the elementary signals received in each mode, T  r̂(t)  r̂(1) (t), r̂(2) (t), · · · , r̂(Np )(t) = Mrx srx (t), (3.4) where s(t) and srx (t) are vectors containing the independent spatial-polarization modes that are active for a specific antenna type and they are related through (3.5) srx (t) = Hch ∗ s(t), where the symbol ∗ indicates matrix convolution, as defined in [36]. The channel Hch , from the transmitter mode vector s(t) to the receiver mode vector srx (t), is the simulated propagation channel developed in chapter 2. 3.2. THE MIMO-OFDM SYSTEM 57 Thus, the mode signal vector r̂(t) at the receiver can be rewritten using equations 3.3, 3.4 and 3.5 as a linear combination of all the transmitted modes, each of which is subjected to the effects of the propagation channel r̂(t) = Mrx Hch ∗ MTtx i(t). (3.6) The coefficients of the linear combination represent the effect of the fading, cross-correlation and depolarization induced by the channel. 3.2 The MIMO-OFDM System Through the combination of MIMO and OFDM (Orthogonal Frequency Division Multiplexing), denoted as MIMO-OFDM, we also achieve orthogonality over the frequency domain by using the Discrete Fourier Transform (DFT) with a Cyclic Prefix (CP) to mitigate the effects of frequency selective and Ts is channels. Assuming a cyclic prefix CP ≥ τd · fs , where fs = T−1 s the symbol time, we can write the received signals as a circular convolution  over the DFT-frame as rm (t) = N  hmn (t)  sn (t) + vm (t), (3.7) n=1 where NDF T = 128 is the size of the DFT, m = 1, · · · , M are the receiving antennas and vm (t) is AWGN. If we have a MIMO antenna system with N transmitting antennas and M receiving antennas, we can then write the signal for sub-channel k in the frequency domain between any pair of transmitting and receiving antennas as rm (k) = N  hmn (k)sn (k) + vm (k), (3.8) n=1 where k denotes each separate subcarrier. If we write equation 3.8 in vector notation we get r(k) = H(k)s(k) + v(k), (3.9) where r(k) is an (M × 1) vector and s(k) is an (N × 1) vector of the received and transmitted signals, respectively. H(k) is the (M ×N ) frequency response matrix H(k) = hmn (k), m = 1, · · · , M and n = 1, · · · , N in 3.7 of the channel between N transmitters and M receivers. The noise in the system v(k) is Chapter 3. Space-Time-Polarization Processing for Capacity 58 Enhancement in HAP/Satellite communication systems an (M × 1) vector assumed to be additive white Gaussian noise. Thus, the correlation matrix of the noise vector v(k) is E{v(k)vH (k)} = σv2 · IM , where σv2 is the variance of the noise and IM is the M × M identity matrix. Since we are using the singular value decomposition (SVD) technique we can now write the channel matrix H(k) as H(k) = U(k)Σ(k)VH (k), (3.10) where Σ(k) is an (M × N ) matrix containing singular values that are larger than zero σ1 (k) ≥ σ2 (k) · · · ≥ σr (k) > 0 where r is the rank of the matrix H(k), and the (M × M ) matrix U(k) and the (N × N ) matrix V(k) contain the corresponding eigenvectors as matrix column vectors. To obtain a diagonalized system we then define y(k) = Σ(k)x(k) + n(k), (3.11) ⎧ ⎨ y(k) = UH (k)r(k) s(k) = V(k)x(k) (3.12) ⎩ n(k) = UH (k)v(k) Since the MIMO-OFDM channels in equation 3.10 are uncorrelated and the correlation of the noise n(k) is E{n(k)nH (k)} = σn2 · IM then we can write the theoretical maximum information capacity of the system [10] as   NDF r T −1  2  σm (k) 2 , (3.13) log2 1 + σxm (k) C= σn2 m=1 where k=0 where σx2m is the variance of the separate uncorrelated input signals in vector x(k). The capacity in equation 3.13 is constrained by the total radiated power from the transmitting antennas, defined as Prad = NDF T −1  r  k=0 m=1 σx2m (k). (3.14) To maximize the total sum of capacities in all the sub-channels we use the so called water-filling technique in which we allocate more power to the sub-channels with high eigenvalues. The optimal water-filling solution [37] is then given by ⎧ 2 σn σ2 2 ⎪ if γ − σ2 n(k) ≥ 0 2 (k) , ⎨ σxm (k) = γ − σm m (3.15) ⎪ 2 ⎩ 2 σn σxm (k) = 0, if γ − σ2 (k) ≤ 0 m 59 3.3. COMPACT ANTENNA ARRAYS where k = 0, · · · , NDFT − 1, m = 1, 2, · · · , r and γ is a pre-defined threshold level of the signal-to-noise ratio in the system and it is dependent on the total transmitted power Prad in equation 3.14. The average signal-to-noise ratio SNRavg in the simulations is calculated as  SNRavg = 10 log10 1 Nactive NDF T −1  k=0 r  σ 2 (k) σx2m (k) m 2 σn m=1  , (3.16) where Nactive is the number of active channels used for which the variance of the input signals σx2m > 0. 3.3 3.3.1 Compact Antenna Arrays Array Configurations The Compact MIMO Antenna Array Configurations each transmit and receive antenna arrangement of the system consists of a special compact MIMO antenna array configuration, which possess a structure of different designs and complexities as shown in figure 3.5. The tested antennas shown in this figure are: the vector element antenna, MIMO-Cube, MIMO-Tetrahedron and MIMO-Octahedron. The detailed description of the structure and analysis of these antennas is presented in the next section. 3.3.2 The Space-Polarization Domain The polarization and antenna radiation pattern of the electromagnetic field can be expressed as a multipole expansion [2, 3] of the field emanating from a virtual sphere enclosing the antenna that is being analyzed. This series expansion consists of weighted orthogonal base functions on the surface of the virtual sphere and allow for a solution to Maxwell’s equations that can be written as (see Appendix A.1), ⎧   j     ⎪ ⎪ ⎨ E = l,m k aE (l, m)(∇ × fl (kr)Xlm ) + aM (l, m)gl (kr)Xlm   (3.17) ⎪ ⎪ j  = 1    ⎩ H l,m aE (l, m)fl (kr)Xlm − k aM (l, m)(∇ × gl (kr)Xlm ) η0 where η0 is the intrinsic impedance of free space. The base functions  lm (ϕ, θ) are orthogonal vector functions of the spherical field  lm (ϕ, θ) = LY X Chapter 3. Space-Time-Polarization Processing for Capacity 60 Enhancement in HAP/Satellite communication systems Figure 3.5: The structure of various compact MIMO antenna array configurations: (top left) vector element antenna, (top right) MIMO-Cube, (bottom left) MIMO-Tetrahedron and (bottom right) MIMO-Octahedron. 3.3. COMPACT ANTENNA ARRAYS 61 in ϕ and θ directions when the far-field of the antenna is projected onto the  = j r×∇ is virtual sphere. Ylm is the scalar spherical harmonic functions and L the angular momentum operator. The radial functions gl and fl in equation 3.17 are spherical Hankel functions representing an outgoing (transmitted) wave or an incoming (received) wave. The weights aE and aM are the corresponding real valued coefficients and will give the gain of each orthogonal function (mode) for a particular electromagnetic far-field pattern, as shown by equation 3.18, ⎧  1 k ⎪ ∗  dΩ ⎪ Ylm (θ, φ) r · E ⎪ ⎨ aE (l, m) ≈ η0 · l(l + 1) fl (kr)  (3.18) k ⎪ ∗ ⎪  ⎪  g (l, m) ≈ − (kr) Y (θ, φ)  r · H dΩ a M l ⎩ lm l(l + 1) By using equation 3.18, we can calculate which modes are active on any arbitrary antenna enveloped by a virtual sphere by knowing the current  the charge distribution ρ and the intrinsic magnetization M  of distribution J, the antenna structure. These modes are theoretically orthogonal to each other and therefore represent independent ports of the antenna. The transmitting channel Htx is then assumed as the linear transformation of the input signal x into the mode domain atx according to atx = Htx x. For the receiving channel we have a similar transformation from the mode domain arx into the output signal y of the system following y = Hrx arx , where atx and arx are vectors containing the mode gains for a specific antenna type. To separate these modes into uncorrelated channels we use singular value decomposition (3.19) H = UΣVH , where U and V are matrices containing the eigenvectors of the antenna and Σ comprise of the antenna gains for independent MIMO subchannels. The orthogonalization of the channel into the independent subchannels is done by multiplying the signal to be transmitted x with the matrix V on the transmitter side of the channel and multiply the received signal y on the receiver side of the channel with the matrix UH y = UH H (Vx) , (3.20) where y is a vector containing the decoded signal from the independent MIMO subchannels and x is a vector of the separate signals to be transmitted through the MIMO channel. Chapter 3. Space-Time-Polarization Processing for Capacity 62 Enhancement in HAP/Satellite communication systems Figure 3.6: The theoretical antenna pattern when the six channels of the vector element antenna are activated. The three omnidirectional antenna beams at elevation angle 0 degrees and azimuth 0 and 90 degrees have both vertical and horizontal polarization. The first compact MIMO antenna array we investigated is known as the vector element antenna [7, 8], see figure 3.5. This antenna consists of three orthogonal electric dipoles forming an electric tripole together with a magnetic tripole formed by three orthogonal loop antennas (magnetic dipoles), which will give a maximum of six independent antenna ports as shown in figure 3.6. The singular values contained in matrix Σ in equation 3.19 for the vector element antenna array are shown in figure 3.7. It can be clearly seen from this figure that we have one very good channel (> -2 dB), four fairly good channels (> -30 dB) and one weak channel (< -40 dB). The second antenna type is the MIMO-Cube [9], which consists of twelve electric dipoles positioned on the twelve edges of a cube as shown in figure 3.5. It can been seen from figure 3.8 that this antenna array has theoretically twelve independent antenna ports. Figure 3.9 show the singular values 63 3.3. COMPACT ANTENNA ARRAYS 0 ï5 relative channel gain [dB] ï10 ï15 ï20 ï25 ï30 ï35 ï40 ï45 1 2 3 4 Channel number 5 6 Figure 3.7: The theoretical antenna gain for each of the six orthogonalized sub channels in the vector element anttena. Chapter 3. Space-Time-Polarization Processing for Capacity 64 Enhancement in HAP/Satellite communication systems Figure 3.8: The theoretical antenna pattern when all twelve channels of the MIMO-Cube antenna are activated. The four antenna beams at elevation angle 0 degrees have vertical linear polarization and the eight beams at elevation ± 45 degrees have horizontal linear polarization. 65 3.3. COMPACT ANTENNA ARRAYS 0 ï10 relative channel gain [dB] ï20 ï30 ï40 ï50 ï60 ï70 ï80 ï90 ï100 1 2 3 4 5 6 7 8 9 Channel number 10 11 12 Figure 3.9: The theoretical antenna gain for each of the twelve orthogonalized sub channels of the MIMO-Cube antenna array. Chapter 3. Space-Time-Polarization Processing for Capacity 66 Enhancement in HAP/Satellite communication systems Figure 3.10: The theoretical antenna pattern when all six channels of the MIMO-Tetrahedron antenna are activated. The three antenna beams at elevation angle 30 degrees have vertical linear polarization and the three beams at elevation -30 degrees have horizontal linear polarization. contained in matrix Σ in equation 3.19 for the MIMO-Cube antenna array. We can clearly see that we have eight fairly strong channels (> -50 dB), one weak channel (< -60 dB) and one very weak channel (< -90 dB). The third compact antenna that we investigated is known as the MIMOTetrahedron [13] as shown in figure 3.5. This antennas has six electric dipoles placed at the six edges of a tetrahedron, and so has theoretically six independent ports as can be seen in figure 3.10. The singular values contained in matrix Σ in equation 3.19 for the MIMO-Tetrahedron antenna array asre shown in figure 3.11. It can be clearly seen from this figure that we have one very good channel (> -2 dB), four fairly good channels (> -32 dB) and one weak channel (< -40 dB). Comparing the sub channel gains of the MIMO-Tetrahedron with the gains of the vector element antenna we can see that the MIMO-Tetrahedron have slightly higher gain in the three strongest 67 3.3. COMPACT ANTENNA ARRAYS 0 ï5 relative channel gain [dB] ï10 ï15 ï20 ï25 ï30 ï35 ï40 ï45 1 2 3 4 Channel number 5 6 Figure 3.11: The theoretical antenna gain for each of the six orthogonalized sub channels of the MIMO-Tetrahedron antenna array. Chapter 3. Space-Time-Polarization Processing for Capacity 68 Enhancement in HAP/Satellite communication systems Figure 3.12: The theoretical antenna pattern when all twelve channels of the MIMO-Octahedron antenna are activated. The six antenna beams at elevation angle 30 degrees have both vertical and horizontal linear polarization and the six beams at elevation -30 degrees also have both vertical and horizontal linear polarization. sub channels than is achieved by the vector element antenna. Finally, the fourth compact antenna we proposed and investigated is a novel array configuration, which we denoted as the MIMO-Octahedron. This antenna consists of twelve electric dipoles positioned in a double tetrahedron geometry, as can be seen in figure 3.5. This design is created by taking two MIMO-Tetrahedron arrays and placing them with one tetrahedron vertex facing a vertex of the other tetrahedron and then rotating one of the tetrahedrons 60 degrees around the axis going through both vertices and finally displace one of the tetrahedron so that they both have the same central point. Theoretically this will give twelve independent ports as can be seen from 3.12. The singular values contained in matrix Σ in equation 3.19 for the MIMO-Octahedron antenna array are shown in figure 3.13. We can clearly 69 3.3. COMPACT ANTENNA ARRAYS 0 ï10 relative channel gain [dB] ï20 ï30 ï40 ï50 ï60 ï70 ï80 ï90 ï100 1 2 3 4 5 6 7 8 Channel number 9 10 11 12 Figure 3.13: The theoretical antenna gain for each of the twelve orthogonalized sub channels of the MIMO-Octahedron antenna array. Chapter 3. Space-Time-Polarization Processing for Capacity 70 Enhancement in HAP/Satellite communication systems see from this figure that we have eigh fairly strong channels (> -50 dB) and four weak channels (< -70 dB). If we compare the MIMO-Octahedron with the MIMO-Cube, we can see that the overall average gain is about the same, however there exist an extremely weak channel in the MIMO-Cube. This observation regarding the MIMO-Cube was also noted in [9]. 3.3.3 Mutual Coupling and Spatial Correlation Assuming that we have a MIMO antenna system with N transmitting antennas and M receiving antennas, the complex envelope of the received signal rm (t) at the receiving compact array after matched filtering can be expressed as the linear convolution rm (t) = N  hnm (t)sn (t − τ ) + vm (t), (3.21) n=1 where m = 1, . . . , M . vm (t) is assumed to be AWGN. Rewriting 3.21 in vector notation results in r = Hs + v, (3.22) where s is the (N × 1) vector containing the transmitted signals from the N transmitting antenna elements and v is the corresponding (N × 1) zero-mean AWGN vector. H in 3.22 is the normalized (N × M ) channel matrix modelled as 1/2 1/2 Zrx (Rrx ) H0 (Rtx ) Ztx , (3.23) H= Crx Ctx where H0 is the channel response without spatial correlation and mutual coupling. Rrx and Rtx are the spatial correlation matrices on the receiving and transmitting side, respectively. The mutual coupling between the elements of the compact antenna array is denoted as Zrx and Ztx normalized by Crx and Ctx , respectively. The mutual coupling is calculated from ⎧  tx −1 ⎨ Ztx = Ztx 0 Z0 + ZL (3.24) ⎩ −1 Zrx = ZL (Zrx + Z ) L 0 where Z0 represents the impedance matrix of the transmitting and receiving compact arrays, ZL is a diagonal matrix containing the source impedance which has been chosen as the complex conjugate of the self impedance given 3.4. DEPOLARIZATION ANALYSIS 71 by the diagonal impedance matrix Z0,ii , and Crx and Ctx are normalizing factors [35]. The spatial correlation matrices Rtx and Rrx are calculated between the antenna element positions and polarization states according to [6] ϕ θ ρp,q = ! ζ κ ϕ θ aq (Θ)a∗p (Θ) sin θp(Θ)dκdζdθdϕ ζ κ |aq (Θ)| sin θp(Θ)dκdζdθdϕ (3.25) 1 ×! ϕ θ ζ κ |ap (Θ)| sin θp(Θ)dκdζdθdϕ where the element p, q of matrix R is the correlation between antenna element p and q. ϕ and θ are the spherical coordinates expressing the spatial domain and ζ and κ are the polarization angle and phase difference, respectively, that account for the effects in polarization domain [6]. In equation 3.25, a(Θ) is the steering vector and p(Θ) is the joint probability distribution function of T the parameter vector Θ = [θ ϕ ζ κ ] , where T denotes a transpose operator. It is assumed that all the parameters are independent of each other and that p(ζ) = u {0, π} and p(κ) = u {−π, π} are uniformly distributed. 3.4 Depolarization Analysis The polarization of a time-harmonic plane-wave is assumed to be the alignment of the electric field component of the TEM plane-wave, which can then be represented by the x− and y−components of the electric field vector  as E  = (Exex + Ey ey ) ejωt . (3.26) E Propagation of a linearly polarized high frequency wave in the ionosphere will experience a rotation of the polarization plane. Depending on the frequency and the length of the path, the amount of rotation can vary from negligible (above 10 GHz) to several rotations (below 1 GHz) [38]. This effect is known as Faraday rotation and is caused by the combined effect of a high electron density and the earth’s magnetic field. In the troposphere, depolarization can be caused by precipitation. All rain drops in a given cloud are affected by similar forces within the cloud which cause a certain degree of alignment between the rain drops [38, 39]. Chapter 3. Space-Time-Polarization Processing for Capacity 72 Enhancement in HAP/Satellite communication systems The polarization of an electromagnetic wave traveling through anisotropic media (e.g. a cloud containing rain and ice particles) is generally altered. Consequently a polarized wave might emerge with some component that is orthogonal to the original polarization state (e.g. vertically polarized signal containing a horizontal component or a Right-Hand Circular Polarized (RHCP) signal containing a component of Left-Hand Circular Polarization (LHCP)). The relationship between these polarization components of the electromagnetic wave is measured by the cross-polar discriminatio (XPD) or the cross-polar isolation (XPI) [38, 39].   E (3.27) XPD = 20 log10 E⊥→   E , (3.28) XPI = 20 log10 E⊥← where E is the amount of the signal that remain in the same polarization state as before, and E⊥→ is the amount of the signal that has scattered out into the opposite orthogonal polarization state. E⊥← is the amount of the opposite orthogonal signal that has scattered into the original signals polarization state. Depolarization from rain is strongly correlated with the rain attenuation and can be calculated from the following empirical formula [38, 39], XPD = a − b log(L), (3.29) where a=35.8 and b=13.4 are reasonable values for frequencies about 10 GHz, and L is the rain attenuation [38, 39]. 3.5 Simulation Results In this section we investigate the capacity improvement resulting from the use of multiple HAP or satellite system employing compact MIMO antenna arrays and compare the results to that obtained from a system without diversity (denoted single-input single-output SISO). In addition, we will also show the effects of mutual coupling and spatial-polarization correlation (calculated by the Finite Element Method) on the capacity of the system. The simulation results are divided according to the used multiple platform (HAP or satellite) and type of channel model employed (referring to table 3.1) for the different scenarios. 73 3.5. SIMULATION RESULTS 8000 Ideal MIMOïCube or ideal MIMOïOctahedron, 12 independent channels and 6 satellites. Ideal Vect. elem. ant. or ideal MIMOïTetrahedron, 6 independent channels and 3 satellites. Single satellite system (SISO), 2 independent channels. 7000 Capacity C [bps] 6000 5000 4000 3000 2000 1000 0 5 10 15 20 Average SNR [dB] 25 30 Figure 3.14: The capacity of the multiple satellite system for the ideal (no mutual coupling or spatial correlation) compact MIMO arrays in figure 3.5. First we compare the capacity for different ideal (no mutual coupling or spatial correlation) compact antenna arrays using satellites in scenarios 1 and 2 (figure 3.14) and HAPs in scenarios 5 and 6 (figure 3.15). The capacity results shown in figure 3.14 are obtained for scenarios 1 and 2 for a system of satellites operating at an altitude of 1200 km and with a separation angle of 20 degrees, and plotted against the average signal-to-noise ratio (SNR) of the system. The elevation angle at both the transmitting and the receiving ground base stations is held at 10 degrees throughout the investigations. Figure 3.15, on the other hand, show the results obtained for scenarios 5 and 6 for a system of HAPs operating at an altitude of 20 km and with a separation angle of 20 degrees, and also plotted against the average signal-tonoise ratio of the system. The elevation angle is held at 10 degrees throughout this investigations as well. It is evident from figure 3.14 and 3.15 that the multiple satellite or multiple HAP diversity system provides superior performance as compared to the Chapter 3. Space-Time-Polarization Processing for Capacity 74 Enhancement in HAP/Satellite communication systems 8000 Ideal MIMOïCube or ideal MIMOïOctahedron, 12 independent channels and 6 HAPs. Ideal Vect. elem. ant. or ideal MIMOïTetrahedron, 6 independent channels and 3 HAPs. Single HAP system (SISO), 2 independent channels. 7000 Capacity C [bps] 6000 5000 4000 3000 2000 1000 0 5 10 15 20 Average SNR [dB] 25 30 Figure 3.15: The capacity of the multiple HAP system for the ideal (no mutual coupling or spatial correlation) compact MIMO arrays in figure 3.5. 3.5. SIMULATION RESULTS 75 single satellite or single HAP case. It is also apparent that the MIMO-Cube antenna or MIMO-Octahedron antenna provides a better capacity than both the MIMO-Tetrahedron and the vector element antenna due to the higher number of acquired platforms (independent channels). Due to the longer distance to the satellites compared to the HAPs the capacity is consequently lower for the satellite system. For example, let us compare the performance of the multiple platform systems (using 3 and 6 platforms) together and with that of the single platform case at an SNR of 20 dB. We can observe that in the multiple satellite system (figure 3.14) that the capacity of 6 satellites is 107% higher than the single satellite system and 59% higher than the 3 satellite system, which in turn is 30% higher than the single satellite system. Performing the same comparison for the multiple HAP system (figure 3.15) yields a capacity of the 6 HAP system that is 158% higher than the single HAP system and 85% higher than the 3 HAP system, which in turn is 39% higher than the single HAP system. Next we investigate the effect of different separation angles between platforms on the capacity for different compact antenna arrays. The maximum capacity, calculated in accordance with equation 3.13, is achieved when there is a spatial-polarization alignment between the modes of the transmitting array and the receiving array. Since the spatial-polarimetric radiation pattern is dependent on the geometrical shape of the compact array, the separation angle where the maximum capacity of the system occurs is also dependent of the geometry of the array and therefore it differs for the different arrays depicted in figure 3.5. For example, figure 3.16 show the effect of the separation angles between platforms on the capacity of the HAP system employing the vector element antenna array. In order to simplify the comparison and show the effect of the separation angle on the performance, we plot the capacity for a fixed SNR of 20 dB for various separation angles (ranging from 0 to 120 degrees in steps of 5 degrees) as shown in figure 3.17. It is clear from this figure that the separation angle between HAPs has a great impact on the system capacity. It is also evident that the optimal separation angle that maximizes the total capacity of the system for an SNR of 20 dB is found to be 20 degrees for the simulated HAP system employing the vector element antenna. Performing similar simulations for the other compact MIMO array configurations (MIMO-Tetrahedron, MIMO-Octahedron and the MIMO-Cube) yield the results shown in figure 3.18 for a fixed SNR of 20 dB and multiple HAPs system (employing 3 or 6 HAPs). From this figure, it is clear that the MIMO-Cube and the vector element antenna array have their maximum capacity at separation angles of 15 and 20 degrees, respectively, while both the Chapter 3. Space-Time-Polarization Processing for Capacity 76 Enhancement in HAP/Satellite communication systems 4000 20° 30° 10° 40° 50° 60° 70° 80° 90° 100° 110° 3500 Capacity C [bps] 3000 2500 2000 1500 1000 500 0 5 10 15 20 Average SNR [dB] 25 30 Figure 3.16: The capacity of the HAP system for various separation angles using the ideal vector element antenna array. MIMO- Tetrahedorn and MIMO-Octahedron have their maximum capacity at 10 degrees. The agreement in optimal separation angle in the MIMOTetrahedorn and MIMO-Octahedron arrays is due to the similar geometry of the arrays, since the MIMO-Octahedron can be seen as two co-located MIMOTetrahedron arrays. It is also clear from figure 3.18 that both the vector element antenna and the MIMO-Cube array are more robust in situations where the platforms are widely spread, and that the MIMO-Tetrahedron and MIMO-Octahedron arrays have better performance in situations where the platforms are positioned close together. We can also observe in figure 3.18 that if the separation angle tends toward 0 degrees the spatial diversity will collapse into a SISO (single platform system). Similar observations were noted for the multiple satellite system. Next, we show the effects of mutual coupling and spatial-polarization correlation (both calculated by the Finite Element Method) on the capacity of the system, and the results are plotted in figures 3.19 and 3.20 for various compact antennas of the multiple satellite system. It is evident from these figures that although the capacity is degraded by correlation and mutual coupling, we still achieve significant gain compared to the single antenna case. 77 3.5. SIMULATION RESULTS 2900 2800 Capacity C [bps] 2700 2600 2500 2400 2300 2200 2100 2000 0 20 40 60 80 100 Separation angle between HAPs e [degrees] 120 Figure 3.17: The capacity for different separation angles using the ideal vector element antenna array at an SNR of 20 dB. Chapter 3. Space-Time-Polarization Processing for Capacity 78 Enhancement in HAP/Satellite communication systems Vector elem. ant. 3 HAPs MIMOïCube ant. 6 HAPs MIMOïTetrahedron ant. 3 HAPs MIMOïOctahedron ant. 6 HAPs 6000 5500 5000 Capacity C [bps] 4500 4000 3500 3000 2500 2000 1500 0 10 20 30 40 Separation angle e [degrees] 50 60 Figure 3.18: The capacity of the multiple HAP system for different separation angles using the ideal compact antenna arrays in figure 3.5, at an SNR of 20 dB. 3.5. SIMULATION RESULTS 79 For example, if we compare the performance in figure 3.19 for an average SNR of 20 dB, we get a 108% higher capacity from the ideal MIMO-Cube antenna than from the ideal MIMO-Tetrahedron antenna, and a 225% higher capacity compared with the non-diversity single HAP system. If we take into account the correlation and the mutual coupling the MIMO-Cube antenna still has a 106% higher capacity than the MIMO-Tetrahedron antenna and a 172% higher capacity than the ideal non-diversity single HAP system. Similar observations were noted for the multiple HAP system. So far, the investigations have been performed with ideal free space loss (FSL) channel model. In scenarios 3, 4, 7 and 8 we use the proposed spacetime-polarization (STP) channel model simulator described in section 3.1.1 to analyze the atmospheric propagation effects on the performance of the multiple platform diversity systems. In the following simulations we set up a multi channel model dominated by LOS components and with weak NLOS components, with a Rice factor of 10, which corresponds to a rural type of environment. For scenarios 3 and 4, the satellites are randomly positioned according to a uniform distribution at altitudes between 1200 and 1500 km and within an angular sector from -60 to +60 degrees. The satellites are moving with a speed of 500 m/s, and the ground stations are stationary. Since this system is using linear polarization the Faraday rotation effect of the ionosphere will have a devastating effect on the polarization de-correlation of the modes if the carrier frequency is below 2 GHz (see chapter 3.4). This could result in total loss of the signal being transmitted. Therefore, a carrier frequency of 10 GHz has been chosen to avoid excessive Faraday rotation. Selecting a 10 GHz carrier frequency then results in a system that is mainly affected by tropospheric effects (see chapter 3.4). Figure 3.21 show the impact on the capacity for different cross-polar discrimination (XPD) values. An XPD = ∞ represents a channel with no depolarization effects and is comparable to scenarios 1 and 2. With moderate precipitation in the troposphere we have an XPD value of 26 dB (calculated according to equation 3.29) which, for example, results in a 23% drop in capacity for an average SNR of 20 dB. With a worse precipitation value (XPD = 16 dB), would result in a 54% drop in capacity. From these results, We can see that precipitation in the troposphere can cause severe degradation in system performance due to the loss of several communication sub channels. At an XPD of 0 dB, we have a total loss of the signal. The corresponding multiple HAP system in scenarios 7 and 8 are setup with a uniform random positioning of the HAPs at altitudes between 17 and Chapter 3. Space-Time-Polarization Processing for Capacity 80 Enhancement in HAP/Satellite communication systems 5000 Ideal Vect.elem.ant. Vect.elem.ant. with mutual coupling. Vect.elem.ant. with mutual coupling and spatial correlation. Ideal single satellite system. 4500 4000 Capacity C [bps] 3500 3000 2500 2000 1500 1000 500 0 5 10 15 20 Avergae SNR [dB] 25 30 25 30 8000 Ideal MIMOïCube ant. MIMOïCube with mutual coupling. MIMOïCube with mutual coupling and spatial correlation. Ideal single satellite system. 7000 Capacity C [bps] 6000 5000 4000 3000 2000 1000 0 5 10 15 20 Average SNR [dB] Figure 3.19: The effect imposed on capacity by mutual coupling between the array elements and by spatial-polarization correlation of the radiation patterns of the array for: (top figure) the vector element antenna array and (bottom figure) MIMO-Cube antenna array. The single antenna system is added in the graph for comparison purposes. 81 3.5. SIMULATION RESULTS 5000 Ideal MIMOïTetrahedron. MIMOïTetrahedron with mutual coupling. MIMOïTetrahedron with mutual coupling and spatial correlation. Ideal single satellite system 4500 4000 Capacity C [bps] 3500 3000 2500 2000 1500 1000 500 0 5 10 15 20 Average SNR [dB] 25 30 25 30 8000 Ideal MIMOïOctahedron. MIMOïOctahedron with mutual coupling. 7000 MIMOïOctahedron with mutual coupling and spatial correlation. Ideal single satellite system. 6000 Capacity C [bps] 5000 4000 3000 2000 1000 0 5 10 15 20 Avergae SNR [dB] Figure 3.20: The effect imposed on capacity by mutual coupling between the array elements and by spatial-polarization correlation of the radiation patterns of the array for: (top figure) the MIMO-Tetrahedron antenna array and (bottom figure) MIMO-Octahedron antenna array. The single antenna system is added in the graph for comparison purposes. Chapter 3. Space-Time-Polarization Processing for Capacity 82 Enhancement in HAP/Satellite communication systems 8000 MIMOïCube with mutual coupling and spatial corr. , XPD = ' MIMOïCube with mutual coupling and spatial corr., XPD = 26 dB MIMOïCube with mutual coupling and spatial corr., XPD = 16 dB. Single satellite system 7000 Capacity C [bps] 6000 5000 4000 3000 2000 1000 0 5 10 15 20 Average SNR [dB] 25 30 Figure 3.21: The effect of depolarization on the MIMO-Cube satellite diversity system compared to the ideal vector element antenna array and ideal single satellite system. 83 3.5. SIMULATION RESULTS 8000 MIMOïCube with mutual coupling and spatial corr. , XPD = ' MIMOïCube with mutual coupling and spatial corr. , XPD = 20 dB MIMOïCube with mutual coupling and spatial corr., XPD = 10 dB Ideal Vect. elem. ant. with 3 HAPs Single HAP system 7000 Capacity C [bps] 6000 5000 4000 3000 2000 1000 0 5 10 15 20 Average SNR [dB] 25 30 Figure 3.22: The effect of depolarization on the MIMO-Cube HAP diversity system compared to the ideal vector element antenna array and ideal single HAP system. 22 km and within an angular sector from -60 to +60 degrees. Performing a similar simulation for a multiple HAP system, we set up a multi channel model dominated by LOS components and with weak NLOS components, with a Rice factor of 10, which corresponds to a rural type of environment. Since HAPs are positioned in the stratosphere below the ionospheric layers there is no Faraday rotation effect. Therefore, a lower carrier frequency of 2.5 GHz has been chosen since the results are only affected by tropospheric effects (see chapter 3.4). Figure 3.21 show the impact on the capacity for various XPD values. As in the satellite scenario, an XPD = ∞ represents a channel with no depolarization effects and is comparable to scenarios 5 and 6. For example, with a fairly-harsh precipitation in the troposphere (XPD = 20 dB) would results in a 30% drop in capacity for an average SNR of 20 dB. With a worse precipitation (XPD 10 dB), would result in a 59% drop in capacity. Thus, it is clear that precipitation in the troposphere can also cause severe degradation in system performance due to the loss of several communication sub channels. In extreme cases, e.g. XPD of 0 dB, will yield a total loss of the signal. Chapter 3. Space-Time-Polarization Processing for Capacity 84 3.6 Enhancement in HAP/Satellite communication systems Conclusions In this chapter we have investigated the capacity enhancement resulting from the use of different compact MIMO antenna arrays in a multiple HAP or multiple satellite in order to enhance the capacity in these systems. Simulation results show that the multiple platform diversity systems utilizing compact MIMO antenna arrays outperform that of a single platform system. It was also shown that the MIMO-Cube and MIMO-Octahedron antenna arrays are superior to the MIMO-Tetrahedron antenna array and the vector element antenna since they have twice the number of independent channels which will result in a higher capacity. Further, a small degradation in capacity is resulted due to the effects of spatial correlation and mutual coupling between the separate antenna array elements of the compact antenna arrays. We have also shown the effects of the separation angle between platforms on system performance, and determined the optimal separation angle that maximizes the total capacity of the system. It has also been shown that MIMO-Cube and vector element antenna arrays are preferred when the platforms are widely separated (> 15 degrees) and that the novel MIMO-Octahedron and MIMO-Tetrahedron are preferred when the platforms are closely positioned (< 15 degrees). We have also presented a novel multi-channel simulator that is taking into account the temporal, spatial and polarization properties affecting the signals. In addition, we have also determined the impact on the total capacity of the proposed platform diversity system. Simulation results have shown that the depolarization will have a severe impact on the performance. Since the compact MIMO-antenna arrays used here only utilizes linear polarization it will experience a devastating depolarization at frequencies lower than 2 GHz, due to Faraday rotation. At frequencies above 10 GHz the Faraday rotation will be negligible, but there is still degradation in performance due to depolarizing precipitation. CHAPTER 4 SPACE-TIME PROCESSING FOR QUALITY IMPROVEMENT OF SHORT RANGE WIRELESS COMMUNICATION LINKS O ver the last decade the world has witnessed explosive growth in the use of wireless mobile communications. Looking around we find users with mobile phones, wireless PDAs, pagers, MP3 players, and wireless headphones to connect to these devices - a small testament of the impact of wireless communications on our daily lives. In addition the burst of new technologies such as Bluetooth and other short-range wireless communications are encouraging the further development of a wide variety of distributed wireless devices [40]. Bluetooth is one of those short range wireless communication technology systems which aims at replacing many proprietary cables that connect one device with another with one universal short-range radio link. Recently, many mobile devices (e.g., mobile phones, PDAs, computer mice) with integrated Bluetooth modules have been introduced. Their wireless technology is used to transfer any kind of data onto these devices. Bluetooth devices operate in the industrial, scientific and medical (ISM) band at 2.4 GHz, and use 79 channels each occupying 1 MHz. The reader is refereed to [41–43] for further information about this technology. Propagation of radio waves inside buildings is a very complicated issue, and it depends significantly on the indoor environment (home, office, factory) and the topography (LOS: line of sight and NLOS: non-line of sight). The Chapter 4. Space-Time Processing for Quality Improvement 86 of Short Range Wireless Communication Links statistics of the indoor channel varies with time due to movements of people and equipment [45]. A survey of indoor propagation measurement and models can be found in [44], and electromagnetic propagation effects in [47]. There are limited investigations in the open literature on the measurements and simulations of multipath wave propagation effects on the performance of live Bluetooth links. In this chapter we present measurement campaigns (signal power, bit error rate and data rate) in indoor office building for LOS and NLOS propagation scenarios and access their effects on the Bluetooth link. These measurements were carried out using various antennas (omni-directional and directive antennas), and we will present comparative analysis to access the potential improvement in system performance gained from the use of directive antennas. We will also show the effect of antenna parameters (gain and efficiency) on the results and the overall impact on the quality and coverage of the Bluetooth link. In addition, in this chapter we will also assess the fading phenomenon by FEM simulation modelling (carried out in the software package COMSOL Multiphysics) [48] of LOS and NLOS propagation scenarios, and use the measurement results and theoretical analysis [49, 50] to confirm our findings. A simple path loss model is derived for the indoor environment and the simulations are also used for assessing the impact on propagation when doors are opened or closed. The spatial properties of wireless communication channels are extremely important in determining the performance of the systems. Thus, there has been great interest in employing space-time signal processing schemes since they can offer a broad range of ways to improve wireless systems performance. For instance, techniques such as Single-Input Multiple-Output (SIMO) and Multiple-Input Multiple-Output (MIMO) can enhance link quality through diversity gain or increase the potential data rate or capacity through multiplexing gain. In the final part of this chapter, we apply these techniques to a Bluetooth system operating over a fading radio channel in a NLOS propagation environment and assess their impact on performance via simulations [51–53]. The organization of this chapter is as follows. In section 4.1 we provide a brief description of the building in the tested indoor office environment and the various types of antennas used in the measurement trials and their related parameters. In section 4.2 we present the results of these measurements. The FEM simulations of the tested environment and the application of space-time processing is featured in section 4.3. Finally, section 4.4 concludes the chapter. 4.1. THE TESTED INDOOR OFFICE ENVIRONMENT 4.1 87 The Tested Indoor Office Environment The measurement trials were performed indoors in typical office environments. In this section we will describe the building structure and material where the measurements took place and later in the results section we show the sensitivity of the Bluetooth link, employing different antenna types, in these indoor environments. Figure 4.1 shows a typical example of office environment which is quite common all over the world. The dimensions of the hallway of the building in this figure are (45 x 1.85 x 2.30) meters. Most doors are mainly made of wood except of the two outer doors, one at each end of the hallway, which are made of metal. The inner walls in the hallway consist of a large single pane window in a wooden frame. The walls between the rooms consist of two plasterboards supported by two vertical steel crossbars and the plasterboards are nailed to vertical wooden crossbars that are situated at regular intervals inside the wall. Mostly all the furniture in the office are made of wood and plastic. The outer walls of the building are made of concrete isolated with thermal material and dual pane windows surrounded by wooden/metal frames. 4.1.1 The Used Antennas The antenna is the interface between the transmitter and the receiver and the propagation medium, and it therefore is a deciding factor in the performance of a radio communication system. To improve and develop the design of Bluetooth antenna, the Bluetooth Special Interest Group (SIG) has left the antenna part as an open door for the antenna manufacturers. In the past few years, the designs of Bluetooth antennas have been developed significantly and since then many companies have entered the Bluetooth antenna market and others had already left it. The Bluetooth radio module has to be connected to an antenna to transport the electromagnetic energy from the radio module to the antenna (transmitter), or from the antenna to the radio module (receiver). In addition, there are three important parameters concerning both the propagation of electromagnetic waves and the definition of the coverage of the wireless devices. These parameters are the receiver sensitivity, output power and antenna gain. The radiation pattern of an antenna could be omnidirectional (a circular pattern with the same radiation in every direction in one plane) or directional. Therefore the radiation pattern in a particular direction determines if the antenna has a directive gain or not. Fixed network devices such as LAN Chapter 4. Space-Time Processing for Quality Improvement 88 of Short Range Wireless Communication Links Figure 4.1: Description of the indoor office environment used in the measurement scenarios for: NLOS (top figure) and LOS (bottom figure). 4.1. THE TESTED INDOOR OFFICE ENVIRONMENT 89 Access Points (LAP) could use antennas that are directed as they are installed. Conversely, mobile devices such as cellular phones, laptops, cameras, etc. need to transmit and receive at any direction and angel. As a consequence, in the choice of an antenna for a product, its position as well as its parameters (gain, efficiency and radiation pattern) should be taken into account and investigated properly. In this chapter, both omnidirectional and directive antenna types have been used and tested. The range of the Bluetooth antenna is much different in practical measurements than the theoretically anticipated range especially in an office environment; this observation will be also revealed in the measurement results section. The popular antenna types for Bluetooth devices are the external dipole, microstrip and planar inverted-F antenna (PIFA). In this chapter the Bluetooth Application Tool Kit has been used in the measurements as we have mentioned above. In order to connect and measure with different antennas by using the Bluetooth Application Tool Kit module which has an originally microstrip PIFA antenna printed on a Printed Circuit Board (PCB) board, a cable with SMA connector has been connected to a feeding point with impedance of 50 Ω as a requirement for each Bluetooth antenna when it would be mounted on the board. The different antenna types used in these test are presented below; the operational frequency range for all antennas is 2.4-2.5 GHz and their nominal feeding impedance is 50 Ω. It is worth mentioning at this point that generic names have been given to the different antennas used in these measurements rather than their specific names. The various tested antennas and their radiation patterns are presented in the appendix. The PIFA antenna used in the Master Bluetooth device has two galvanic contacts, one to the earth and the other as a feeding point with impedance of 50 Ω. The structure of the PIFA antenna is optimized for small size requirements, large bandwidth and efficient gain. The size of the PIFA antenna is (25 × 7) mm. The Half Wave Model 1 antenna (Appendix figure B.1) relies on a reflection formed wave between the active element and a conductive plane. It is a big directional antenna. The gain value of this antenna is 9.2 dBi and its efficiency is 95%. Because of its large size, this antenna can be used as an external antenna for some applications like a printer server and measuring instruments. The return loss, which has been measured with a network analyzer, is 14.4 dB. The Half Wave Model 2 antenna (Appendix figure B.2) is an external antenna which was supplied with an adjustable radiator angle. This antenna could take different positions (vertical, horizontal, etc.). The Half Wave Model Chapter 4. Space-Time Processing for Quality Improvement 90 of Short Range Wireless Communication Links 2 antenna is characterized by a radiation pattern which is almost the same at all directions (omnidirectional). The gain value of this antenna is 1.6 dBi, the efficiency is 75% and the return loss is 15 dB. The Quart Wave Model 1 antenna (Appendix figure B.5) has a small size of (18.2 × 3.9 × 1.6) mm, and it has surface-mounted embedded antenna. It can be integrated into PC cards, mobile phones, access points and Bluetooth enabled devices. It is a linearly polarized antenna with a peak gain of 2 dBi. The Quart Wave Model 2 antenna (Appendix figure B.4) is also small in size (21 × 4 × 3) mm and can be used as an embedded antenna for Bluetooth enabled devices. The gain value of this antenna is 4.1 dBi, its efficiency value is 68% and the return loss is 10.784 dB. The radiation pattern of the Quart Wave Model 2 antenna is not omnidirectional. The Half Wave Model 3 antenna (Appendix figure B.3) has relatively small size (27 × 8 × 3) mm and can be used both as an embedded antenna and an external antenna for Bluetooth enabled devices. The radiation pattern of this antenna indicates that the Half Wave Model 3 antenna is not an omnidirectional antenna. The gain value of this antenna is 4.0 dBi, its efficiency is 62% and the return loss is 13.46 dB. 4.1.2 The Measurements Setup Measurement campaigns were conducted so that we can get an understanding of how the signal power, BER and the data rate are affected by NLOS and LOS propagation scenarios for the different Bluetooth antennas that have been used in the indoor office environment. The antennas used in these measurement trials and their parameters have been described in the previous section. One room (back room marked with a dot) and part of the hallway were used in the measurements to provide NLOS and LOS scenarios between the two Bluetooth devices/antennas, respectively, as shown in figure 4.1. A PC is connected to a Bluetooth device with PIFA antenna, have been used as a stationary Bluetooth device (Master). Another PC with a Bluetooth device (Slave), was rolled along the hallway in 1 m interval following the dotted line in figure 4.1. The various used antennas, which are described in the previous section, were replaced alternately on the Slave side. In this chapter, the Receiver Signal Strength Indicator (RSSI) is used in the measurements; this term and signal power has been used interchangeably here. The Bluetooth RSSI measurement compares the received signal power with two threshold levels, which define the Golden Receive Power Range [41]. Note that all the results for signal power measurements were registered after measuring it 10 4.2. RESULTS OF THE MEASUREMENTS 91 times to ensure that a stable signal is being measured. For the fast fading dip identification, the measured return value of RSSI was flickering (or hopping) from 0 dB to -20 dB and back again to 0 dB and so on (i.e., a stable result couldn’t be measured). Note that the door in the back room, where the master was placed for NLOS scenario, was open and other doors in the hallway were also open during the measurements. In addition, people in the office were allowed to move freely during the measurements, and the results of these measurements were registered after a successful data transmission. For the NLOS measurement scenario all the measurements have been started at the range of 3 meters (see figure 4.1) in order to avoid the direct LOS path. 4.2 Results of the Measurements Antennas that are able to direct the transmitted and received signals’ energy are of great interest for future wireless communication systems. The directivity implies reduced transmit power and interference and hence potential for increased capacity, quality and range. In this section we present the measurement trails using different directive antennas and compare with isotropic antenna for NLOS and LOS propagation scenarios described in the previous section. The results of tree types of measurement trails (signal power, bit error rate and data rate) will be presented in this section. The RSSI or signal power measurement results are shown in figure 4.2. It is evident from this figure that a significant reduction in signal power is achieved with the gradual increase of both the distance and the number of the obstacles between the Master and the Slave along the dotted line in figure 4.1. Increasing the distance ever further will ultimately produce a break in transmission; that is a disconnection between the radio modules at different distances depending on the parameters (gain and efficiency) of the different used antennas and the propagation scenario. This is the reason why the Half Wave Model 1 antenna (9.2 dBi, 95%) has the highest signal power and best range (19 meters) while the Half Wave Model 3 antenna (4 dBi, 62%) has the lowest signal power and range (9 meters). The results of the other antennas are intermediate between the results of the above two mentioned antennas. Note that a successful data transmission was impossible after the coverage range of each antenna shown in figure 4.2. The most important distance in this scenario is at 10 meters which is the anticipated range of the Bluetooth class 3 modules used in these measurements. Chapter 4. Space-Time Processing for Quality Improvement 92 of Short Range Wireless Communication Links An interesting observation in NLOS scenario is the reception of stable (or constant) signal power level (in some distances for all the used antennas) in spite of increasing the distance between the Master and the Slave. This can be clearly seen from the RSSI results in figure 4.2 for example at the distance from 9-12 meters, and will be verified to a certain extent by the FEM model although in the simulation we can observe some fluctuations. An important observation that can be made from figure 4.2 regarding LOS scenario is that the signal still exists in the hallway much farther beyond the operating range of 10 meters (see for example Half Wave Model 1 ). This phenomenon could be explained by the tunnelling effect where the hallway acts as a waveguide to the reflected radio waves from the walls along the hallway. Hence the increased coverage ranges as compared to NLOS scenario. In figure 4.3 we show the results of BER measurements for the different antennas. BER is defined as the number of errors in the system that occurs within a given sequence of bits. For example, a BER of 10−4 means that in average one bit out of 10000 bits is corrupted. Generally, the BER becomes higher by increasing the distance between the transmitter and the receiver, and by increasing the number of obstacles in the communications path. However, the effect of fast fading on the measurement results is evident from the rapid fluctuation of the measured BER values for all antennas as shown in figure 4.3. Again, the Half Wave Model 1 antenna provided the best results (lowest BER values) among the other used antennas, which is clearly related to its high gain and efficiency parameters. For NLOS scenario in figure 4.3a, the highest BER value of 1.964% was obtained by the Half Wave Model 3 antenna at a distance of 12 m, while the lowest BER value of 0.378% (at the same distance) was obtained by the Half Wave Model 1 antenna, see figurefig:BER. The BER results of the other antennas were in between the above mentioned values. On the other hand, for LOS scenario in figure 4.3b, the results of BER measurements show a minimum value of 0.0% (no errors) and a maximum value of 0.905%, see figure 4.3. In other words, the BER is lower in LOS as compared to NLOS scenario as expected. Again, the Half Wave Model 1 antenna has the best results (lowest BER values) among the other used antennas, which is clearly related to its high gain and efficiency parameters. Finally, the results of the data rate measurements are plotted in figure 4.4. From these plots we notice only a very slight reduction of the Bluetooth link data rates with increasing the distance. The data rate results are also in agreement with the pattern of the BER results in figure 4.3; that is the higher the BER value, the lower data rate that can be achieved and vice versa. This 4.2. RESULTS OF THE MEASUREMENTS 93 Figure 4.2: The signal power measurements results for: NLOS (top figure) and LOS (bottom figure). The RSSI generally drops with increasing the distance between the Master and the Slave. Chapter 4. Space-Time Processing for Quality Improvement 94 of Short Range Wireless Communication Links Figure 4.3: The BER measurement results for: NLOS (top figure) and LOS (bottom figure). The BER increases with distance and the rapid fluctuations are due to fast fading. 4.3. FEM SIMULATIONS 95 can be clearly seen in the distance of 12 m for NLOS scenario, where the highest data rate value of about 172.2 kbps, see figure 4.4 was obtained by the Half Wave Model 1 antenna and the lowest data rate value of 169.4 kbps, see figure 4.4 was obtained by the Half Wave Model 3 antenna. The results of the Quart Wave Model 2, Quart Wave Model 1 and Half Wave Model 3 antennas has followed a similar pattern by giving intermediate data rate values as was the case for RSSI and BER scenarios. A similar pattern of results (not shown) were obtained from LOS scenario. Figure 4.4: The data rate measurement results for NLOS. Only a slight drop in data rates is obtained with increasing distance between the transmitter and receiver. 4.3 4.3.1 FEM Simulations The Simulated Indoor Model The simulation of the radio waves is done using the Finite Element Method (FEM) which is numerically solving Maxwell’s field equations for the electromagnetic field. Here we are using the software package COMSOL Multiphysics Chapter 4. Space-Time Processing for Quality Improvement 96 of Short Range Wireless Communication Links for the finite element calculations. In a macroscopic environment we can write Maxwell’s field equations as:   = − ∂B ∇×E ∂t   = J + ∂ D ∇×H ∂t ρ  ∇·D = ε  =0 ∇·B (4.1)  Fourier transforming these equations and solving for either the electric E  field or the magnetic H field we obtain the time-harmonic Helmholtz equation:  (here is shown the solution of the electric field E)  = jωµJ  + ω 2 εµE ∇2 E (4.2) For simplicity, the vector arguments (r, ω) and the term e j ωt are omitted here and for the remainder of this chapter. The field in our model is source-free everywhere except inside the transmitting antenna element where we have the current Iz from the transmitter with an even distribution over the cross-section area Aant of the  r, ω): antenna element giving the current density J( ⎧ ⎨ ẑ · Iz (r, ω) , inside the antenna element  Aant (4.3) J(r, ω) ⎩ 0, elsewhere Assuming that the model does not contain any material with magnetic properties we can describe the electric properties of the different materials as a complex valued dielectric parameter εc defined as:   σ (4.4) εc = ε r − j ωε0 where εr is the relative permittivity and σ is the conductivity of the material for a specific angular frequency ω. In table 4.1 is shown the different materials with corresponding permittivity and conductivity used in our model [48]. In this model we assume that these parameters are independent of time. 4.3. FEM SIMULATIONS Material Glass Plaster board Brick 97 Table 4.1: Material properties. Dielectric constant εr Conductivity σ [mS/m] 4.2 1 · 10−11 2.27 0.18 4.44 1 The full 3D model of the office environment, used in the simulations, is shown in figure 4.5 and in figure 4.6 the 2D projection of this partial building can be viewed and compared to the real floor plan of the office building shown in figure 4.1. Figure 4.5: The simplified office model obtained from transferring the real floor plan in figure 4.1 into a CAD (Computer Aided Design) program. 4.3.2 FEM Simulation Results In this section we present the FEM simulations of the indoor office environment. The simulations were performed at the frequency 2.402 GHz. The simulations are divided into four cases which differ in the position of the transmitting antenna and whether or not the doors along the hallway are opened or closed. The antenna is either placed in the corridor or in the top right office room as shown in figure 4.1. In order to obtain a complete comparison between the FEM simulation results and the measurements data, we have divided the simulations into a line of sight (LOS) environment (figure 4.7) and a non line of sight (NLOS) environment (figure 4.8). The Chapter 4. Space-Time Processing for Quality Improvement 98 of Short Range Wireless Communication Links Figure 4.6: The 2D projection of the model in figure 4.5. collection of data from the simulated model has been done along the same path that the real measurements (figure 4.1) were done. These paths can be seen in figures 4.1, 4.7 and 4.8 marked by dashed arrows. In figures 4.7 and 4.8 the simulation results are shown as the two dimensional power distribution of the transmitted signal. " calculated as the time averaged magnitude " This is " " of the Poynting vector "S (r, ω)", where r = (x, y, z). The rapid change in power over a very short distance in space is caused by superposition of the reflected, diffracted, refracted and scattered components of the wave with itself. This power level variation is shown by the two dimensional fading pattern in figures 4.7 and 4.8, for LOS and NLOS propagation scenarios, respectively. These figures clearly illustrate the tunneling effect phenomenon along the hallway and give an indication about the range of operation. In addition, the figures also confirm the predominance of the tunneling effect and the extended range in LOS as compared to NLOS propagation scenario. These observations are in agreement with the measurement results presented in the previous section. If we collect signal power data (by measurements or simulations) along the path indicated by the arrows in figures 4.7 and 4.8 we obtain an average signal power or received signal strength indicator (RSSI) as shown in figures 4.10 and 4.9 for NLOS and LOS, respectively. Since the FEM simulations were done assuming an omnidirectional antenna, the power profile should be 4.3. FEM SIMULATIONS 99 Figure 4.7: FEM simulations showing the two dimensional power distribution inside the office environment for a LOS scenario with all the doors along the hallway closed (top figure) or opened (bottom figure). The transmitter is positioned at the coordinate (x=5m; y=2m). Chapter 4. Space-Time Processing for Quality Improvement 100 of Short Range Wireless Communication Links Figure 4.8: FEM simulations showing the two dimensional power distribution inside the office environment for a NLOS scenario with all the doors along the hallway closed (top figure) or opened (bottom figure). The transmitter is positioned at the coordinate (x=7.5m; y=26.5m). 4.3. FEM SIMULATIONS 101 compared with measurement results using an omnidirectional antenna as presented in figures 4.9 and 4.10. It is evident from these figures that the real measurements and simulation results show reasonable agreement for both propagation scenarios. Since the simulated model is experimentally confirmed, and this is a weakstationary problem with a narrow band time-harmonic signal, it is in this case sufficient to describe the channel parameters as a Ntx × Nrx complex-valued matrix H ⎤ ⎡ H12 ··· H1Nrx H11 ⎢ H21 H22 H2Nrx ⎥ ⎥ ⎢ ⎥ ⎢ . .. ⎥ H H H H=⎢ (4.5) 31 32 3Nrx ⎥ ⎢ ⎥ ⎢ .. .. .. ⎦ ⎣ . . . HNtx 1 HNtx 2 · · · HNtx N rx These complex-valued numbers Hij describe the amplitude and phase due to the distance between the different combinations of transmitting and receiving antennas. In order to validate the results presented above we compare these results with the theoretical statistics of the signal as shown in figure 4.11. It can be seen that the probability distribution (density function) of the signal in the NLOS scenario is close to a Rayleigh distribution (top plot in figure 4.11) which is to be expected in a NLOS environment. On the other hand, we obtain a Rice probability distribution (bottom plot in figure 4.11) with a Rice-factor K ≈ 1.4 for LOS scenario. By inspecting figures 4.9 and 4.10 and observing the changes in the signal strength, we can assess the impact on propagation when the doors along the hallway are either opened or closed. An interesting observation from these simulations is that we have a change in power levels when the doors of the offices are opened compared to when they are closed; this observation of ”door state” is also confirmed by real measurements done in [54]. This effect however, does not seem to be as prominent in the NLOS scenario since the signal strength is only less affected by the status of the doors. To model the NLOS path loss of the office environment, we sample the simulated received signal strength along paths leading away from the transmitting antenna. The NLOS paths (a, b and c) that have been analyzed are shown in figure 4.12. A power-distance law [55] is developed using a regression model fitted to the sampled data from the simulation (see figure 4.13). The path loss exponent Chapter 4. Space-Time Processing for Quality Improvement 102 of Short Range Wireless Communication Links 4 Simulated RSSI (Doors opened) Simulated RSSI (Doors closed) Measured RSSI (Doors opened) 2 0 Average power [dB] ï2 ï4 ï6 ï8 ï10 ï12 ï14 ï16 0 5 10 15 Distance [m] 20 25 Figure 4.9: Power profile for LOS scenario using: measurement data for an omnidirectional antenna and simulated data when doors along the hallway are opened or closed. 103 4.3. FEM SIMULATIONS 0 Simulated RSSI (Doors opened) Simulated RSSI (Doors closed) Measured RSSI (Doors opened) ï2 Average power [dB] ï4 ï6 ï8 ï10 ï12 ï14 ï16 0 2 4 6 8 Distance [m] 10 12 14 Figure 4.10: Power profile for NLOS scenario using: measurement data for an omnidirectional antenna and simulated data when doors along the hallway are opened or closed. Chapter 4. Space-Time Processing for Quality Improvement 104 of Short Range Wireless Communication Links Distribution of signal simulated NLOS data theoretical Rayleigh distribution 0.6 Probability 0.5 0.4 0.3 0.2 0.1 0 0 1 2 3 4 Signal strength 5 6 7 Distrbution of signal simulated LOS data theoretical Rice distribution 0.45 0.4 Probability 0.35 0.3 0.25 0.2 0.15 0.1 0.05 0 1 2 3 4 Signal strength 5 6 7 Figure 4.11: (top plot) The probability distribution of the simulated NLOS data and the theoretical Rayleigh distribution, and (bottom plot) the probability distribution of the simulated LOS data and the theoretical Rice distribution with a Rice factor of approximately 1.4. 4.3. FEM SIMULATIONS 105 a b c Figure 4.12: NLOS propagation scenario where the arrows show the three analyzed paths: a) path going through the upper office walls, b) path along the corridor, and c) path going through the lower office walls. β is estimated using the least squares method. The model is described as the logarithmic loss L(d) at the distance d from the transmitting antenna according to (4.6) L(d) = L(d0 ) − 10β log10 (d) where d0 is a distance of reference. The path loss exponent β is then compared between different scenarios to discern the behaviour of the propagating field in different indoor environments. As a reference, β = 2, represents the wellknown free space exponent value. By taking the mean value of 100 estimated values of β simulated along the corridor (see figure 4.12) we find β ≈ 1.71 with a standard deviation of σ ≈ 0.05 which is due to the tunneling effect of the corridor. For the path following the upper arrow in figure 4.12, the same analysis yields β ≈ 4.43 with a standard deviation of σ ≈ 0.02 and for the lower path we have β ≈ 3.14 with a standard deviation of σ ≈ 0.02. These estimates of the path loss exponent β are consistent with findings chaptered in the literature [39, 55]. Next, we investigate the improvement in system performance resulting from diversity gain and multiplexing gain in NLOS scenarios of a system employing multiple transmit/receive antennas with different combining techniques. The simulations of the single-input multiple-output (SIMO) and Chapter 4. Space-Time Processing for Quality Improvement 106 of Short Range Wireless Communication Links ï95 Simulated data Regression model ï100 Received Power [dBW] ï105 ï110 ï115 ï120 ï125 ï130 ï135 0 5 10 15 20 Distance from the transmitter [m] 25 Figure 4.13: An example of a regression model (red) fitted to the sampled data from the simulations (blue). 107 4.3. FEM SIMULATIONS multiple-input multiple-output (MIMO) system were done along the same paths of the indoor office building shown in figure 4.12 and at a high signal to noise ratio (SNR) of 50 dB in order to get a fair comparison. Multiple-antenna channels provide spatial diversity, which can be used to improve the reliability of the link. The basic idea is to supply to the receiver multiple independently faded replicas of the same information symbol, so that the probability of all signal components fading simultaneously is reduced. To illustrate this point for a SIMO system, we show in figure 4.14 the simulated received signal power from five receiver antennas separated by half a wavelength. These five received signals are combined to give an overall improvement of the system by taking advantage of the diversity gain achieved through multiple receiving antennas, as shown in figure 4.15. This figure shows the diversity gain for a SIMO system (employing 1 transmitting antenna and 5 receiving antennas) for three different types of combining methods: Selection Combining (SC), Equal Gain Combining (EGC) and Maximum Ratio Combining (MRC) [52, 53]. Compared with the single antenna system we can see that SC will give around 1-2 dB gain, EGC results in about 2-3 dB while MRC improves the signal by 6-8 dB. 5 0 Rx Power level [dB] ï5 ï10 ï15 ï20 ï25 ï30 0 5 10 15 20 Distance from transmitter along xïaxis [m] 25 30 Figure 4.14: The power profile from five receiving antenna elements separated by half a wavelength. To further show that multiple antennas provide a robust source of diversity Chapter 4. Space-Time Processing for Quality Improvement 108 of Short Range Wireless Communication Links 10 Seletion combining Equal combining Maximum ratio combining Single antenna Received Power level [dB] 5 0 ï5 ï10 ï15 ï20 ï25 ï30 0 5 10 15 20 25 Distance from transmitter along xïaxis [m] 30 Figure 4.15: Improvement of the received signal due to different receiver diversity combining methods. 109 4.3. FEM SIMULATIONS gain in NLOS channels, we perform simulations using an increasing number of antenna elements at the receiver. From figure 4.16 we can clearly see that even a few extra antennas at the receiver will result in a noticeable increase the diversity gain (e.g. two extra antennas will give a 0.65, 1.87 and 3.23 dB diversity gain respectively for the three examples of combining methods). These results suggest that using multiple receiver antennas will improve the indoor coverage of the transmission, especially if we use the Maximum ratio or Equal gain combining methods. Antenna receive diversity (SIMO) 14 Theoretical Maximum Ratio Equal gain Selection Diversity gain Gdiv [dB] 12 10 8 6 4 2 0 0 5 10 15 Number of receiver antennas N 20 Figure 4.16: The receiver diversity gain obtained by a SIMO system with three different combining methods. Finally, we consider the use of diversity (or multiple antennas) at both the transmitter and receiver, respectively, giving rise to a MIMO system. The MIMO system simulation has been analyzed for both spatial diversity and spatial multiplexing schemes. That is to say, a MIMO system can provide two types of gain: diversity gain and spatial multiplexing gain. In the case of spatial diversity, the procedure is the same as for the SIMO system described above and a MRC of the antennas output is used to provide maximum diversity gain. In the case of spatial multiplexing, we create separate uncorrelated sub channels to send data in parallel data streams Chapter 4. Space-Time Processing for Quality Improvement 110 of Short Range Wireless Communication Links which can then be interpreted as an increase of the total channel capacity or an SNR improvement of the total channel. In this analysis we use the SNR and compare it with the SNR enhancement resulting from the diversity gain. If the SNR of the channel is improved the path loss exponent β will accordingly decrease. 5 4.5 Path loss exponent ` 4 3.5 3 2.5 2 1.5 1 2 3 4 5 6 7 8 9 10 Number of antennas at the transmitter and receiver respectively [Ntx × Nrx] Figure 4.17: Showing the decrease of β in proportion to the size of the Ntx × Nrx MIMO antenna system. In this analysis we have the same number of antennas both on the transmitting and receiving side. Figure 4.17 shows the path loss exponent versus the size of the antenna array for the three paths shown in figure 4.12. The blue, red and green data points and graphs corresponds to path a, b and c, respectively, in figure 4.12. From this figure it is clear that increasing the number of antennas will result in a decrease of the path loss exponent for the MIMO diversity system (solid lines and  for data points). The decrease in β is in the order of -0.14 per each added antenna except in path c where the decrease is -0.52 per each added antenna. In the case of spatial multiplexing (dashed lines and  for data points) we have a decrease in β by -0.78 per each added antenna except along path a where we only have a decrease of -0.34 per each added antenna. The spatial multiplexing system offers at least a 50% improvement in the path loss 4.4. CONCLUSIONS 111 exponent compared to the diversity system. It should also be stressed that the number of antenna elements to be used would depend on many factors such as the physical size of the different devices, power requirements, complexity and cost restrictions imposed by manufacturing. 4.4 Conclusions In this chapter we investigated the wave propagation effects of a shortrange wireless device operating at 2.4 GHz in an indoor office environment. The investigations were carried out using measurement trials and FEM propagation modelling for NLOS and LOS propagation scenarios. The measurement trails and simulations have shown good agreement. This was also confirmed by comparison with the theoretical statistical probability distribution of the signal in both scenarios. A power-distance exponential propagation law was found to be sufficient to describe the propagation both for corridors (propagation exponent β ≈ 1.66 − 1.76) and through office walls (propagation exponent β ≈ 3.12 − 4.45). The FEM simulations were also used for assessing the influence on propagation when doors are opened or closed. The simulation results have shown a power loss in LOS scenario when the doors of the offices are opened compared to when they are closed and that this effect does not appear to be prominent in the NLOS scenario. We have also investigated a SIMO antenna diversity system utilizing different combining techniques and a MIMO antenna system using spatial diversity and spatial multiplexing schemes to improve the performance over a fading radio channel in a NLOS propagation environment. Our results show a substantial gain would be achieved using a MIMO spatial multiplexing system. It also shows that even a SIMO scheme would offer a considerable diversity gain and improvement in system performance. However, more investigations are necessary to better understand the path loss behaviour in a multiple antenna system. Chapter 4. Space-Time Processing for Quality Improvement 112 of Short Range Wireless Communication Links CHAPTER 5 POWER CONSTRAINED SPACE-TIME PROCESSING FOR SUPPRESSION OF ELECTROMAGNETIC FIELDS T here have been several studies done, with conflicting results, on the effects of cell-phone radiation on the human body [56–58]. The amount of radiation emitted from most cell phones is very minute. However, given the close proximity of the phone to the head, it is entirely possible for the radiation to cause harm. If you want to be on the safe side, the easiest way to minimize the radiation you are exposed to is to position the antenna as far from your head as possible. Utilizing a hands-free kit, a car-kit antenna or a cell phone whose antenna is even a couple of inches farther from the head can do this most effectively. This chapter makes a contribution to that discussion by proposing a new approach employing adaptive active control algorithms combined with a Multiple-Input Multiple-Output (MIMO) antenna system to suppress the electromagnetic field at a certain volume in space. Active methods for attenuating acoustic pressure fields have been successfully used in many applications. In this paper we investigate if these methods can be applied to an electromagnetic field in an attempt to lower the power density at a specified volume in space. The cancelling out of a signal can be achieved by employing the principle of superposition. For example, if two signals are superimposed, they will add either constructively or destructively. The objective of our study is to investigate the possibility of applying adaptive active control algorithms Chapter 5. Power Constrained Space-Time Processing 114 for Suppression of Electromagnetic Fields with the goal of reducing the electromagnetic field power density at a specific volume using the superposition principle and MIMO antenna system. Initially, the application we evaluate is a model of a mobile phone equipped with one ordinary transmitting antenna and a number of actuator-antennas which purpose is to cancel out the electromagnetic field at a specific volume in space (e.g. at the human head) [59–63]using power level information obtained by an sensor antenna array. Later, we investigate the effects of the size and number of MIMO antenna elements on the performance of the system [59, 61]. It is worth stressing at this point that the purpose of this MIMO system is not to improve the capacity or quality of transmission between the mobile unit and base station, but to predict the channel response or sense the radiated field which can then be controlled by using the active control algorithms. For this purpose, a class of algorithms called Filtered-X [76, 77, 80], which are well known from the area of acoustic noise cancellation are employed and evaluated to assess their behaviour and performance in this electromagnetic type of environment. By constraining these adaptive algorithms we also try to make the total output power level transmitted by the antenna elements, locked to a predefined value. This power constraint is achieved through the use of a quadratic constraint on the active control algorithms [60–63]. The modelling of the antenna elements and the electromagnetic field calculations are performed using the simulation package FEMLAB (currently COMSOL Multiphysics) [64, 65]. This software is also used in combination with MATLAB to implement and test the adaptive algorithms used to control the electromagnetic field. The operating carrier frequency used in the initial investigation is 900 MHz (a wave length λ of approximately 0.33 m). Later, we test the algorithms at different carrier frequencies (e.g., other GSM bands and UMTS) [59]. The organisation of this chapter is as follows. In section 5.1, we present the FEMLAB MIMO antenna model. In section 5.2, the different unconstrained adaptive algorithms used to suppress the power density of the electromagnetic field are presented. Simulation results comparing these different algorithms are shown in section 5.3. The constrained solution of the output power is presented in section 5.4. Simulation results investigating the effects of the different MIMO antenna system parameters including the operating frequency are analysed and presented in section 5.5. Finally, section 5.6 concludes the chapter and presents further research ideas. 5.1. THE MODEL 5.1 5.1.1 115 The Model The FEM model The application used in this chapter is a three-dimensional (3D) model of a physical system consisting of eight vertical antenna elements and of a human head, a two-dimensional representation of the 3D model is shown in figures 5.1 and 5.2, respectively. The simulation of the radio waves is performed numerically by using the finite element method (FEM) in COMSOL Multiphysics software package for solving the electromagnetic field equations. Figure 5.1: 2D model representing the tested physical system. In a simple medium where we have no external sources except inside the transmitting antenna elements, we can write Maxwell’s equations in timeharmonic form as:  = j ωB  ∇×E  = µJ − j ωµD  ∇×B  =ρ ∇·D (5.1)  =0 ∇·B (5.4) (5.2) (5.3) where the vector arguments and the term e −j ωt are omitted for simplicity. To solve the electric field with the current density in the antenna as the  from equation 5.2 and input source we eliminate the magnetic flux field B get:    = j ωµJ  − ω 2 εµE (5.5) ∇× ∇×E Chapter 5. Power Constrained Space-Time Processing 116 for Suppression of Electromagnetic Fields meter Boundary meter Figure 5.2: The FEM representation of the 2D model in figure 5.1. The outer boundary is set to a radius of 1 meter to limit the FEM solution.  = 0 and we get If it is assumed that there are no free charges, then ∇ · E the inhomogeneous Helmholz’s equation:  = −j ωµJ  + ω 2 εµE ∇2 E (5.6) The parameters denoted by ε (permittivity), µ (permeability)and σ (conductivity) define the electromagnetic properties of the different materials in the model. To model materials that contain both conductive and dielectric properties, a complex valued permittivity εc is defined:   σ (5.7) εc = ε r − j ωε0 where σ is the conductivity and εr is the relative permittivity of the material when there is an incident time-harmonic wave with an angular frequency ω. Several authors have suggested permittivity and conductivity values of the human brain tissues as a function of frequency (examples in [72–74]). The 5.1. THE MODEL 117 data have been assessed through measurements or by deriving values from the intensity levels of magnetic resonance images (MRI) and thermographies, or by theoretical analysis. This variety of methods give a wide range of geometrical and dielectric properties of the brain tissue. The most common data was published 1957 by Schwan [71]. Schwan and other authors validated these values up to microwave frequencies [72, 73], and proposed analytical expressions derived from Debye’s model of molecular dipole moment in dispersive materials. The standardization seems to converge on data published by Gabriel [74]. For simplicity an average of the electric properties of the brain and skull is used here; for example at a frequency of 900 MHz the following parameters are used εr =45.805496 σ =0.766504[S/m] (5.8) (5.9) These values are based on the 4-Cole-Cole equation as described in [74]. The antenna elements are assumed to be made out of copper and will have the following electric properties εr =1, since this is no dielectric material σ =5.99 · 10 .[S/m] 7 (5.10) (5.11) If we assume that there are no ferromagnetic materials in this FEM model, it will be sufficient to set the permeability equal to the free space permeability µ = µ0 . The finite element method requires that the modelled area is finite and therefore it needs an outer boundary as is clearly shown in figure 5.2. In order to simulate an electromagnetic wave travelling out towards infinity using this model, it is necessary to define the outer boundary of the modelled area so that it does not reflect any signal back towards the antennas (i.e. total absorption at the outer boundary):    outside = 0  inside − D (5.12) n · D where n is the normal vector of the boundary pointing outwards, and since it is a virtual boundary there are no surface charges or currents. This will then lead to a Neuman type of boundary condition:  ∂D  = −j (n · k) D ∂n (5.13) Chapter 5. Power Constrained Space-Time Processing 118 for Suppression of Electromagnetic Fields √ where k = ω εµ. In the model created here the wave will be very close to orthogonal against the boundary in all directions so there will be no significant reflection of the  = εE  we will get the boundary equation: wave. Since D     !   =0  − ω n2x + n2y + n2z εµ E (5.14) n · ∇E  When the time-harmonic solution of the electric field components E(x, y, z) is calculated (see figure 5.3), COMSOL Multiphysics solves the other fields  the magnetic automatically using Maxwell’s equations to get the magnetic H,   flux density B and the electric displacement D fields, respectively. Figure 5.3: The numerical solution to the electric field problem.   y, z) and The E(x, y, z) is then used to calculate the Poynting vector S(x, the time averaged power density. In this case with a stationary wave, this 5.1. THE MODEL vector can be defined as [68]: % & # $  =  1E  ×H ∗ , S 2 119 (5.15) where · denotes a time average. Figure 5.4: A surface plot showing the calculated magnitude of the power density based on the electric field solution. The best way to visualize the power density # $ is by using a two-dimensional  in decibels as illustrated in surface plot to show the magnitude of S figure 5.4.  Further, from the numerical FEM solution E(x, y, z) we can also calculate the maximum specific absorption rate (SAR) value according to SAR = σ ·  2 |E| ρ (5.16) where σ is the conductivity and ρ is the density of the material. The SAR value calculated in the simulations is the maximum SAR value in each point Chapter 5. Power Constrained Space-Time Processing 120 for Suppression of Electromagnetic Fields inside the human head. This value is not the same as the value used in the standards for mobile telephones, which is the mean value of equation 5.16 taken over 10 gram of tissue. The SAR limit recommended by the International Commission of NonIonizing Radiation Protection (ICNIRP) is 2 W/kg averaged over 10 gram of tissue. Thus to fulfill this limit with certainty we need to have a maximum SAR below 2 W/kg. 5.1.2 The MIMO model To reduce the electromagnetic field within a certain volume in the FEMmodelled space, a MIMO radio channel is modelled in order to compensate for the spatial displacement. In this chapter, the FEM simulation program ”COMSOL Multiphysics” is used to simulate the physical MIMO antenna system, which (initially in this Section) consists of 3 transmitting antennas and 5 receiving antennas as shown in figure 5.1. The spacing between the antenna elements used in this application is 0.02m  λ; thus this arrangement can not be seen as an ordinary beamformer as the antenna elements are working in the radiated near-field. The input signals to this system are three separate currents in a complex-valued phasor notation, one for each transmitting antenna. The simulated output current from the 5 receiving antennas form a complex-valued data vector denoted as the error signal vector of the system. The centre antenna T2 (see figure 5.1) is transmitting the signal that we want to cancel (it acts as the antenna on any ordinary mobile telephone) and the two flank transmitter antennas T1 and T3 (see figure 5.1) are denoted as actuator-antennas, which will be used to reduce the signal from the antenna T2 at some specified volume. By changing the amplitudes and phases of the currents assigned to the three transmitting antennas it is possible to control the transmitted power from the separate antenna elements. The calculated time-harmonic electromagnetic wave in the model will then generate a current density inside the receiving antenna elements. According to Ampere’s law for a time-harmonic wave in a simple conductive media we have the following equation:   = j ωµεc E ∇×B (5.17) The total output current Iout from each receiving antenna element can be calculated by integrating both sides over the cross section area S of the 121 5.1. THE MODEL antenna element:  Iout = jωε0 σ εr − j ε0 ω    dS E (5.18) S The result from each antenna element is then stored in a complex-valued data vector e. If we have a system of three transmitter antennas and five receiver antennas the transmitter antenna in the middle (T2 ) (see figure 5.1) is the one we want to cancel, then the two flanking transmitter antennas are denoted as the actuator-antennas (T1 , T3 ). Since the simulated model is experimentally confirmed to be linear, and this is a weak-stationary problem with a monochromatic time-harmonic signal, it is in this case sufficient to describe the parameters as a 5×3 complex-valued matrix H: ⎤ ⎡ H11 (ω) H12 (ω) H13 (ω) ⎢ H21 (ω) H22 (ω) H23 (ω) ⎥ ⎥ ⎢ ⎥ (5.19) H=⎢ ⎢ H31 (ω) H32 (ω) H33 (ω) ⎥ ⎣ H41 (ω) H42 (ω) H43 (ω) ⎦ H51 (ω) H52 (ω) H53 (ω) These complex-valued numbers Hij describe the amplitude and phase due to the distance between the different combinations of transmitting and receiving antennas. The general mathematical MIMO model is shown in figure 5.5. Figure 5.5: The general mathematical MIMO model of the entire antenna system. Chapter 5. Power Constrained Space-Time Processing 122 for Suppression of Electromagnetic Fields Each column in H represents the time-harmonic frequency response functions between one of the transmitting antennas and each of the receiving antennas. The superimposed signals received by the antenna array, constitutes a vector e with five complex-valued elements:  T (5.20) e = e1 e2 e3 e4 e5 If we divide the matrix H is into two separate complex-valued matrices (F and g) as shown in figure 5.6, we get: ' F = [H1 H3 ] = and g = H2 =  F11 F12 g1 F21 F22 g2 g3 F31 F32 F41 F42 g4 g5 F51 F52 T (T (5.21) (5.22) The two columns in F represent the frequency response functions of the actuator -antennas and are denoted as the forward channels. The vector g is denoted as the direct channel and represents the frequency response function of the antenna with the signal we want to cancel out. The total noise of the model is described by vector v, and can be modelled as a complex-valued additive white Gaussian noise vector. The vector e is the combined signals and noise received from the antenna array as shown in figure 5.6. Figure 5.6: Block diagram of the antenna system described as two channels. If the carrier signal transmitted through the direct channel g is to be suppressed at the receiving antenna array, a phase-shifted and amplified copy of the same carrier signal could be transmitted through the forward channels 123 5.1. THE MODEL to superimpose the signal in the direct channel. This could be achieved by incorporating a filter w which would allow control over the signals going through the forward channels as shown in figure 5.7. v s g x w + e Control F Algorithm Figure 5.7: Model of the direct channel g, and the forward channels F controlled by the filter w. To achieve the best possible attenuation in energy sense, the total energy output ξ of the signal e at the receiving antennas must be as low as possible. The minimum energy with respect to the filter w is:     2 (5.23) min ξ = min E |e| = min E eH e w w w where H denotes a conjugate transpose. With the noise v included in the system, the residual error signal e in equation 5.20 is given by: e = sg + sFw + v (5.24) If the input signal s and the noise v are assumed to be uncorrelated, then the mean energy can be written as: ξ = rd + wH p + pH w + wH RF w + rv (5.25) where RF is the covariance matrix of the forward channels, p is the crosscorrelation between the direct channel and the forward channels, rd and rv are the signal power of the direct channel and the noise, respectively. The minimum energy ξmin is found by differentiating ξ with respect to the complex conjugate of filter coefficients w∗ and then setting the derivative equal to zero: (5.26) ∇w∗ ξ = 0 ⇔ p + RF w = 0 Chapter 5. Power Constrained Space-Time Processing 124 for Suppression of Electromagnetic Fields wopt = −R−1 F p (5.27) This is the Least Mean Square (LMS) solution to the problem and is the optimal solution in mean energy sense. Figure 5.9 shows the surface plot of the power density solution when the filter coefficients controlling the signals going through the forward channels are the optimal least mean square coefficients wopt obtained from equation 5.27. Figure 5.8: The power density in the model with no optimization. 5.2. THE ADAPTIVE ALGORITHMS 125 Figure 5.9: The power density in the model when the optimal filter coefficients wopt are used. 5.2 The Adaptive Algorithms The least mean square solution in equation 5.25 describes a quadratic form in the complex valued w-domain, and there is only one optimum point. The gradient of the quadratic performance surface will be evaluated with respect to the conjugate filter coefficients: −∇w∗ ξ . This will give the local steepest descent direction towards the minimum point of the performance surface. To give some idea of how these complex valued filter coefficients move toward the minimum point, the magnitude of the filter coefficients are plotted in figure 5.10 and in figures 5.11-5.14 and figure 5.18 for the other different adaptive algorithms. If the point (w0 , w1 ) in figure 5.10 has the energy value ξ, then a new point in direction of the negative gradient vector must be closer to the minimum point of the surface. So this will give an iterative update equation of the filter-coefficients as: (5.28) wn+1 = wn + (−∇w∗ ξ(n)) The mean-energy ξ of the error function can according to equations 5.23 Chapter 5. Power Constrained Space-Time Processing 126 for Suppression of Electromagnetic Fields Figure 5.10: The quadratic performance surface where the energy ξ is depicted as equivalued closed contour-curves. and 5.24 be expressed as:     = E eH e =   H E (sg + sFw + v) e ξ=E |e| 2 (5.29) If we differentiate equation 5.29 with respect to the conjugate of the filter coefficients w∗ we get the gradient of the mean energy:   (5.30) −∇w∗ ξ = −E FH s∗ e Define FH s∗ ≡ XH , we get:   −∇w∗ ξ = E −XH e (5.31) The expected value is generally unknown, so this can be estimated by a sample mean instead; that is: ˆ w∗ ξ = −XH e −∇ ˆ denotes the estimated gradient. where ∇ (5.32) 127 5.2. THE ADAPTIVE ALGORITHMS If this is substituted into the weight-updating equation 5.28 we get: wn+1 = wn + µ (∇w∗ ξ(n)) = wn − µXH e (5.33) This is the so-called Filtered-X LMS [76, 80] (FX-LMS), since X is the input signal filtered through the forward channels F. The step-length µ in FX-LMS is a constant value and therefore the stability range and convergence rate will change with the change of input power as: 0<µ< 2 Tr (RF ) (5.34) To get around the change of convergence rate, consider that: ( ' 5 5 2 ∗ |F | Fm1 Fm2 2 m=1 RF = s∗ FH Fs = |s| · 5m=1 m1 ∗ 5 2 m=1 Fm1 Fm2 m=1 |Fm2 | (5.35) Then the trace of the matrix RF will be: 2 Tr (RF ) = |s| 5  2 |Fm2 | |Fm1 | 2 (5.36) m=1 where m designates the five different receiving antennas. The above range for convergence (equation 5.34) can then be written as: 0<µ< 2 |s| 2 5 2 m=1 |Fm2 | |Fm1 | 2 (5.37) If we introduce a new step-length parameter β (0 < β < 2) and normalize by the trace of the matrix RF , we get: µ= 2 |s| 5 m=1 β 2 |Fm2 | |Fm1 | 2 (5.38) Then the range of the step-length will be fixed within the range 0 < β < 2. If this substitution is made in the FX-LMS weight-updating algorithm (equation 5.33), we get the Normalized FX-LMS algorithm:   XH n e (5.39) wn+1 = wn + β α + Tr (RF ) where α is a noise regulating parameter if the elements of RF are small [76,80]. Chapter 5. Power Constrained Space-Time Processing 128 for Suppression of Electromagnetic Fields Another approach to an adaptive algorithm is by using the optimal least mean square solution from equation 5.27 in combination with the gradient vector of the quadratic performance surface [76, 80]: ∇ξ = RF w + p (5.40) If we multiply both sides of the gradient by R−1 F , we get: R−1 F ∇ξ = w − wopt (5.41) Rearrange equation 5.41 into an iterative equation where wn = w is the present position (or iteration) and wn+1 = wopt is the next position, we get: wn+1 = wn − R−1 F ∇n ξ (5.42) If the expression of the gradient vector is inserted into equation 5.42 we obtain: (5.43) wn+1 = wn − R−1 F (RF wn + p) = wopt This is the FX-Newton algorithm and its iterative equation moves from any arbitrary point wn on the performance surface to the minimum point in one single step. This can be clearly seen in figure 5.11 for a signal-to-noise ratio (SNR) of 30 dB. If the noise level is high (i.e., low SNR), this can give a very erratic search of the minimum point with a large misadjustment (i.e. noise) as illustrated in figure 5.12. One approach to smooth the misadjustment noise is by using a step-length variable µ as a smoothing regulator: wn+1 = wn − µR−1 F (RF wn + p) (5.44) where 0 < µ < 1. This solution is still going to give an erratic search with a large misadjustment, unless a very small step-length is used which will also slow down the rate of convergence. However, if the gradient vector (RF wn + p) is estimated by the sample mean as was done in the FX-LMS algorithm [76], we get:   ˆ w∗ ξ = Ê XH e = XH e (5.45) −∇ whereˆdenotes an estimation. 5.2. THE ADAPTIVE ALGORITHMS 129 Figure 5.11: The Newton algorithm finds the minimum point in one step. SNR = 30 dB. Using equation 5.45, the new weight update equation is given by:   ˆ wH ξ (n) = wn − µR−1 XH ∇ (5.46) wn+1 = wn − µR−1 n e F F n This is the so-called FX-Newton/LMS algorithm, which is a compromise between the two adaptive approaches. This will result in a greatly enhanced smoothing of the gradient-noise as can be seen from figure 5.13. The main problem with both the FX-Newton and the FX-Newton/LMS algorithms is the need to calculate the inverse of the covariance matrix, which is computationally inefficient. However, if the diagonal elements of the covariance matrix RF are large compared to the off-diagonal values, then the covariance matrix can be estimated from: R̂F ≈ diag {RF } (5.47) By inserting this estimate into the weight updating equation and using a separate step-length for each matrix element, we get: wn+1 = wn − MXH n e (5.48) Chapter 5. Power Constrained Space-Time Processing 130 for Suppression of Electromagnetic Fields Figure 5.12: The erratic search of the Newton algorithm when the noise level is high. SNR = 10 dB. ) where M=  5µ1 |s|2 · m=1 |Fm1 | 0 * 0 2  5µ2 |s|2 · m=1 |Fm2 | 2 Equation 5.48 is known as the Actuator Individual Normalized FX-LMS algorithm [77]. If the eigenvalues of RF are disparate, then the Actuator Individual Normalized FX-LMS will outperform the Normalized FX-LMS since each filter weight will be controlled and normalized separately. On the other hand, if the eigenvalues of the covariance matrix roughly have the same value, then the Normalized FX-LMS and the Actuator Individual Normalized FX-LMS behave in a similar way as can be seen from figure 5.14. 5.3 Simulation Results In the previous section we presented the different adaptive algorithms to suppress the power density of the electromagnetic field and thereby decreasing the maximum SAR value inside the human head. These algorithms are 5.3. SIMULATION RESULTS 131 Figure 5.13: This plot clearly shows why the Newton/LMS algorithm (the green trace) is preferable to the ordinary relaxed Newton algorithm (the red trace) when a high noise level is present in the estimation of the gradient vector. SNR = 10 dB. unconstrained; that is there is no control over the total output power from the mobile phone. In chapter 5.4, the constrained solution will be presented. In this section we evaluate and compare the different unconstrained adaptive algorithms. The ordinary FX-LMS algorithm is the simplest to implement of the evaluated algorithms, but this algorithm has some disadvantages when the input signal is non-stationary. The Normalized FX-LMS algorithm normalizes the input signal with its signal power, resulting in a more robust algorithm at the expense of higher computational complexity. Another approach to the adaptive search is Newton’s method where it is possible to solve the problem in one single step under ideal conditions. This single-step algorithm, however, is very sensitive to noise and is therefore impractical. To improve the noise insensitivity of the Newton algorithm, a gradient vector estimate is used to smooth the algorithm. This algorithm is called the FX-Newton/LMS. Both the FX-Newton and FX-Newton/LMS algorithms require a matrix inversion of the covariance matrix, resulting in high computational complexity. The Chapter 5. Power Constrained Space-Time Processing 132 for Suppression of Electromagnetic Fields Figure 5.14: A comparison between the Actuator Individual Normalized FXLMS and the FX-Newton/LMS. Since the eigenvalues of RF and of diag (RF ) are roughly the same the two algorithms will behave in a similar fashion. Actuator Individual Normalized FX-LMS algorithm only uses the diagonal of the covariance matrix to simplify the problem of calculating the inverse of the covariance matrix. From the above discussion and by testing the algorithms by simulations, it was concluded that the Normalized FX-LMS and the Actuator Individual Normalized FX-LMS are the preferred algorithms since they are both robust and noise-insensitive. Figure 5.15 shows the calculated maximum SAR level inside the human head relative to the maximum SAR level of a single transmitting antenna for both adaptive algorithms. The figure also show the corresponding maximum SAR level attained by employing a passive five element reflector and the least mean square solution which is used as a benchmark for comparisons. The amount of SAR attenuation achieved by the least mean square solution is approximately 12 dB relative to the maximum SAR level produced by a single antenna system (i.e., by using the direct transmitting antenna only, as shown in figure 5.1). It is clear from figure 5.15 that the adaptive algorithms after convergence give about 10 dB more attenuation compared to using the 133 5.4. POWER CONSTRAINTS maximum Specific Absorption Rate SAR [W/kg] 4 a 3.5 3 2.5 b 2 1.5 1 d c 0.5 e 0 0 10 20 30 40 50 Iterations Figure 5.15: The maximum SAR level inside the human head. Plots (from top to bottom): a) One transmitting antenna only. b) 5 passive sensor elements as a passive reflector. c) FX-LMS. d) Actuator Individual FX-NLMS. e) Least Mean Square solution. five receiving antenna elements as a passive reflector. It can also be seen that the Actuator Individual FX-NLMS converges about 40% faster than the FXNLMS towards the least mean square solution, since each diagonal element of the covariance matrix is normalized separately. Finally, in figure 5.16 we show the power density field for one transmitting antenna with five passive reflector elements, and in in figure 5.17 three transmitting antennas tuned to the least mean square solution (i.e., the adaptive algorithms after convergence), respectively. It is clearly evident from this surface plot that the electromagnetic power density field inside the head is lower in the adaptive algorithms case. 5.4 Power Constraints In the previous sections we presented the different unconstrained adaptive algorithms to suppress the power density of the electromagnetic field and their respective simulation results. There is however a major drawback with these Chapter 5. Power Constrained Space-Time Processing 134 for Suppression of Electromagnetic Fields Figure 5.16: Power density surface plot inside the human head (referring to figure 5.1) using one active transmitting antenna with five passive reflector elements (plot b in figure 5.15). adaptive algorithms: that is although the SAR is attenuated by approximately 5 dB (as shown in plots c-e in figure 5.15) inside the human head, there is no control over the total output power from the mobile phone. This means that the total output power changes when the filter adapts, which is unfortunate since the magnitude of the total output power from the mobile phone depends on the distance from the base station. For example, if we take the case of three transmitting antennas and five receiving antennas, this would result in an increase of the total output power by approximately 20% (although this still gives a suppression of 5 dB inside the human head). However, with some other antenna spacing the mobile phone might lose the connection when the adaptive suppression filter converges towards the optimum value. To alleviate this problem, some form of power constraint [60] could be used on the minimization process; that is:   (5.49) min rd + wH p + pH w + wH RF w + rv wH 2 2 subject to: |sw| + |s| = C, C∈ 135 5.4. POWER CONSTRAINTS where the symbol  denotes a real number. This optimization problem can then be solved by forming a Lagrange equation [81] defined as:   (5.50) L (w, λ) = wH RF w + wH p + pH w − λ C − s∗ wH ws − s∗ s By differentiating this Lagrange equation and setting it to zero, we get a suboptimal solution of w which is dependent on the variable λ: ∇wH L (w, λ) = 0 2 ⇔ RF wco + p + λ |s| wco = 0   2 RF + λ |s| I wco = −p (5.51) (5.52) where wco denote the constrained values of the filter coefficients. If we multiply equation 5.52 by R−1 F we get:   2 I + λ |s| R−1 wco = −R−1 (5.53) F F p The right hand side of equation 5.53 is the unconstrained optimal solution wopt which was derived earlier in this chapter (see equation 5.27). Using this information and rearranging equation 5.53, we get: −1  2 wopt (5.54) wco = − I + λ |s| R−1 F It can be clearly seen from equation 5.54 that it is now possible to adjust the unconstrained solution by using a diagonal loading of the covariance matrix. The parameter λ can be chosen so that equation 5.54 satisfies the constraint. Unfortunately there are no closed form solutions for the optimal value of the loading variable λ. However, equation 5.54 can be simplified by employing a Maclaurin expansion of the first term on the right hand side, for values of λ that are close to zero. If we use the first two terms of the MacLaurin expansion (see equation 5.55), it is possible to derive an approximate expression where we only need to perform a single matrix inversion operation: −1  2 2 ≈ I − λ |s| R−1 (5.55) I + λ |s| R−1 F F When this approximation is substituted into the solution of the constrained minimization, we get the constrained values of the filter coefficients as: wco = −wopt − λ |s| R−1 F wopt 2 (5.56) Chapter 5. Power Constrained Space-Time Processing 136 for Suppression of Electromagnetic Fields To find out which value of λ we need, the constraint (equation 5.57) should be solved for the value of the constrained filter coefficients wco and the required power constraint level C: 2 2 |swco | + |s| = C (5.57) This will yield a quadratic equation which has the following solution: +     H 2  H  C H w 2 ·  wopt q ± q − 4 · qH q wopt + 1 − −2 ·  wopt opt |s|2 λ= 2 H 2 · |s| q q (5.58) where q = R−1 w . opt F So, by setting the constraining power level C and using the unconstrained optimal values of the filter coefficients wopt , we can now use equation 5.58 to calculate what the value of λ should be. This value is then inserted into equation 5.56 in order to calculate the constrained filter coefficients wco , which (for convenience) is re-stated again here: wco = −wopt − λ |s| R−1 F wopt 2 (5.59) As an example, if the constrained filter coefficients of equation 5.59 are used in the iterative FX-LMS adaptive algorithms, it can be seen in figure 5.18 that it will converge at the non-optimal solution that satisfy the constraint and has the shortest distance to the unconstrained optimal point. The convergence of this non-optimal constrained least square solution for the Actuator Individual FX-NLMS can also be observed in figure 5.19 and in figure 5.20 is shown the maximum specific absorption rate (SAR) inside the human head when the Actuator Individual FX-NLMS algorithm have reached the constrained least square solution. In figure 5.20 and figure 5.21 we show the effect of using an adaptive algorithm with a power constraint imposed on the solution. The purpose of this constraint is to allow for the minimum SAR value inside the human head while keeping the radiated power from the antenna system at a level consistent with the specified radiated output power from a mobile phone. The adaptive algorithm used in figures 5.20, figure 5.21 and figure 5.19 is the Actuator Individual Normalized FX-LMS algorithm with an imposed constraint according to equation 5.59. 5.5. THE EFFECTS OF MIMO ANTENNA PARAMETERS AND CARRIER FREQUENCY 137 5.5 The Effects of MIMO Antenna Parameters and Carrier Frequency The Least Mean Square solution obtained in chapter 5.3 is the optimal solution in energy sense for this problem. This particular solution (figure 5.4) is only valid assuming the position of each element does not change. However, there might be positions of the antenna elements that are more favorable with respect to the power density and SAR level inside the head. By changing the spacing of the antenna elements during calculations of the attenuated SAR level inside the human head we will investigate if there exist some optimal spacing between the different antenna elements. In this FEM model setup we assume three degrees of freedom (DOF), as shown in figure 5.22. The spacing between the sensor elements, denoted ∆y, the distance (d) between the sensor element array (the receiving elements) and the actuator element array (the transmitting elements). The third DOF is the spacing between the actuator elements, denoted ∆a. In the first analysis we look at how the spacing of the sensor elements and the distance between the transmitter and receiver antennas affect the SAR level inside the head, see figure 5.23. It is clear from figure 5.23 that the farther apart the transmitter and receiver antennas are located the lower the SAR level is inside the head. This is due to the increase of the distance (d) (see figure 5.22) between the transmitter and receiver antennas. An increase of this distance will also increase the distance between the transmitter antennas and the head which will decrease the SAR level inside the head. By analyzing figure 5.23 we can see that the two-dimensional cost function J (∆y, d) is flattening out at a distance d of approximately 25 cm. The spacing between the sensor elements (receiving elements) at the distance d=25 cm should be approximately 5 cm. With this spacing the sensor element array will cover a larger portion of the head. By using these values as a good approximation of the optimal displacement of the actuator elements and the distance between the sensor elements this would result in an SAR attenuation of approximately 7 dB. Using these values as a starting point, figure 5.24 is showing how the separation of the actuator antenna elements ∆a affects the SAR level of the cost function J (∆y, d) inside the head. From figure 5.24 we can see that the attenuation inside the head will increase as the spacing between the actuator elements decrease. This is a consequence of the electromagnetic waves being transmitted from almost the Chapter 5. Power Constrained Space-Time Processing 138 for Suppression of Electromagnetic Fields same point in space. The theoretical extreme of this is to place all actuator antennas in the exact same position, which will give a complete cancellation of the waves and would give a zero power and SAR level inside the head. According to this analysis we need a MIMO antenna system that has a spacing of 5 cm between the sensor elements and a spacing of 3 cm between the actuator elements. The distance between the sensor elements and actuator elements should be about 25 cm or more. This would result in a MIMO antenna system with a size of approximately 25 by 20 cm which is not practical to place on top of a mobile phone. However, we foresee many applications where this size would be practical. Studying figure 5.23 and figure 5.24 we observe that if the original positions of the antenna elements, with an actuator antenna spacing of 2 cm is used and we increase the spacing of the sensor elements from 2 cm to 3 cm we would get an extra 2 dB SAR attenuation inside the head compared to the original positioning of the antenna elements in figure 5.1. We have also investigated the impact on the systems performance as a result of changing the number of antenna elements in the actuator and sensor arrays. In these simulations we have calculated the least mean square solution as a function of the number of antenna elements in the actuator array M and the sensor array N. Figure 5.25 shows, as expected, a decrease in the SAR level inside the head as long as every new added sensor element cover more of the head. Although, when the sensor array extends outside the length of the human head we attain no further improvement in the attenuation. Another interesting observation from figure 5.25 is that if the number of actuator elements is larger than the number of sensor elements the system becomes unstable. Finally, we investigate the effect of the carrier frequency on the system performance. The suppression of the electromagnetic field inside the head so far in this chapter has been analyzed at the GSM frequency band centered at 900 MHz. Therefore, it would be interesting to investigate the effect of using this system at higher carrier frequencies in order to evaluate its performance at other GSM bands and the UMTS frequency band. In this experiment, we sweep the carrier frequency of the simulated system between 500 MHz and 2.5 GHz and the results can be viewed in figure 5.26. From this figure it can be clearly seen that we have a minimum point at the carrier frequency of 950 MHz. This optimum frequency is dependent on the type and size of the different antenna elements. It can also be noted from figure 5.26 that the SAR attenuation of the power level at GSM/UMTS frequencies does not differ by more than 1-2 dB’s. 5.6. CONCLUSIONS 5.6 139 Conclusions In this chapter we have presented a FEM model which solves the partial differential equation of an electromagnetic field and simulated the physical MIMO antenna system which is controlled by various adaptive signal processing algorithms in order to suppress the field at a certain volume in space. We have also presented the solution for constraining the total output power of the system to a predefined level. In addition, we have investigated the effects of the size and number of MIMO antenna elements on the performance of the system and also tested the algorithms at different carrier frequencies. The SAR attenuation levels achieved from these simulations suggest the possibility of using an active antenna system for the reduction of electromagnetic field density. However, our result also show some limitations associated with implementing these antenna arrays in mobile phones, for which further research is needed to find practical solutions. In addition, we foresee other applications where this array size and arrangement would be suitable for practical implementation. Chapter 5. Power Constrained Space-Time Processing 140 for Suppression of Electromagnetic Fields Figure 5.17: Power density surface plot inside the human head (referring to figure 5.1) using three transmitting antennas tuned to the least mean square solution (plot e in 5.15). 141 5.6. CONCLUSIONS The Quadratic Performance Surface 0.8 Absolute Value of Weight w0 0.7 0.6 0.5 0.4 0.3 0.2 0.1 0.1 0.2 0.3 0.4 0.5 0.6 Absolute Value of Weight w1 0.7 0.8 Figure 5.18: An example of using the power constraint in combination with the FX-LMS algorithm. The red trace shows the convergence of the unconstrained filter coefficients. In the green trace we have a constraint that allows for half the power needed to reach the optimal point. Chapter 5. Power Constrained Space-Time Processing 142 for Suppression of Electromagnetic Fields maximum Specific Absorption Rate SAR [W/kg] 4 a 3.5 3 2.5 b 2 1.5 1 d f c 0.5 e 0 0 10 20 30 40 50 Iterations Figure 5.19: The maximum SAR level inside the human head. Plots (from top to bottom): a) One transmitting antenna only. b) 5 passive sensor elements as a passive reflector. c) FX-LMS. d) Actuator Individual FX-NLMS. e) Least Mean Square solution. f) Actuator Individual FX-NLMS with constraint. The average total power level inside the human head -35 dB Minimum without constraint The average total power level inside the human head -26 dB Minimum with constraint } Total antenna output at optimal attenuation with a constraint ~0.26 dB Figure 5.20: Power density suface plots inside the human head. Comparing the attenuation of electromagntic energy inside the human head and the radiated power from the antenna system without constraint (bottom left figure) and with a constraint (bottom right figure). All three figures have the distance in x and y directions measured in meters. { } Total antenna output at optimal attenuation ~1.1 dB Total antenna output power normalized to 0 dB Before minimization 5.6. CONCLUSIONS 143 for Suppression of Electromagnetic Fields 144 Chapter 5. Power Constrained Space-Time Processing Figure 5.21: The same results as in figure 5.20, but the three plots are zoomed out to show more of the far-field. Comparing the attenuation of electromagntic energy inside the human head and the radiated power from the antenna system without constraint (bottom left figure) and with a constraint (bottom right figure). All three figures have the distance in x and y directions measured in meters. 145 5.6. CONCLUSIONS R1 T1 Dy R3 T2 T3 R2 Da R4 R5 TM RN d Figure 5.22: The MIMO system showing the three variables of the antenna displacement. Chapter 5. Power Constrained Space-Time Processing 146 for Suppression of Electromagnetic Fields Distance between Tx and Rx antenna elements d [cm] SAR 50 45 2 40 35 1.5 30 25 1 20 15 0.5 10 5 2 4 6 8 10 12 14 16 Spacing of sensor elements 6y [cm] 18 20 Figure 5.23: The maximum SAR level inside the head as a 2-dimensional cost function J (∆y, d) with respect to the spacing between the sensor elements and the distance between the transmitting and receiving antennas. These SAR levels refer to a system with N=5 sensor elements and M=2 actuator elements. 147 5.6. CONCLUSIONS 1.4 Specific Absorption Rate SAR [W/kg] 1.3 1.2 1.1 1 0.9 0.8 0.7 0.6 0.5 0.4 0 5 10 15 Spacing of sensor elements 6y [cm] 20 Figure 5.24: The effect of increasing the spacing ∆a between the actuator antenna elements. This result was calculated with a sensor array spacing of ∆y = 5 cm and a separation between the sensor array and the actuator array of d = 25 cm. Chapter 5. Power Constrained Space-Time Processing 148 Specific Absorption Rate SAR [W/kg] for Suppression of Electromagnetic Fields 10 8 6 4 2 0 2 0 4 5 6 10 8 10 15 Number of Sensor array eleme Number of Actuator array elements Figure 5.25: The maximum SAR level inside the human head as a function of the number of elements in the actuator and sensor array. 149 5.6. CONCLUSIONS 5.5 Specific Absorption Rate SAR [W/kg] 5 4.5 4 3.5 3 2.5 2 1.5 1 500 1000 1500 Frequency f [MHz] 2000 2500 Figure 5.26: The change in SAR level inside the human head at different carrier frequencies. This simulation was done with a sensor array spacing of ∆y = 3 cm and a distance between the sensor array and the actuator array of d = 3 cm. Chapter 5. Power Constrained Space-Time Processing 150 for Suppression of Electromagnetic Fields CHAPTER 6 SPACE-TIME PROCESSING FOR INTERFERENCE MITIGATION IN HAP WCDMA SYSTEMS T hird generation mobile systems are gradually being deployed in many developed countries in hotspot areas. However, owing to the amount of new infrastructures required, it will still be some time before 3G is ubiquitous, especially in developing countries. One possible cost effective solution for deployments in these areas is to use High Altitude Platforms (HAPs) [82–90] for delivering 3G (WCDMA) communications services over a wide coverage area [36, 91, 92, 94, 95]. HAPs are either airships or planes that will operate in the stratosphere, 17-22 km above the ground. This unique position offers a significant link budget advantage compared with satellites and much wider coverage area than conventional terrestrial cellular systems. Such platforms will have a rapid roll-out capability and the ability to serve a large number of users, using considerably less communications infrastructure than required by a terrestrial network [82]. In order to aid the eventual deployment of HAPs the ITU has allocated spectrum in the 3G bands for HAPs [96], as well as in the mm-wave bands for broadband services at around 48GHz worldwide [97] and 31/28GHz for certain Asian countries [98]. Spectrum reuse is important in all wireless communications systems. Cellular solutions for HAPs have been examined in [99, 100] , specifically addressing the antenna beam characteristics required to produce an efficient cellular structure on the ground, and the effect of antenna sidelobe levels on Chapter 6. Space-Time Processing for Interference 152 Mitigation in HAP WCDMA Systems channel reuse plans [100]. HAPs will have relatively loose station-keeping characteristics compared with satellites, and the effects of platform drift on a cellular structure and the resulting inter-cell handover requirements have been investigated [101]. Cellular resource management strategies have also been developed for HAP use [102]. Configurations of multiple HAPs can also reuse the spectrum. They can be used to deliver contiguous coverage and must take into account coexistence requirements [36, 92]. A technique not widely known is their ability to serve the same coverage area reusing the spectrum to allow capacity enhancement. Such a technique has already been examined for TDMA/FDMA systems [34,103,104]. In order to achieve the required reduction in interference needed to permit spectrum reuse, the highly directional user antenna is used to spatially discriminate between the HAPs. The degree of bandwidth reuse and resulting capacity gain is dependent on several factors, in particular the number of platforms and the user antenna sidelobe levels. An alternative method of enhancement is to apply space-time diversity techniques, such as Single-Input Multiple-Output (SIMO) receive diversity or Multiple-Input Multiple-Output (MIMO) diversity, to improve the spectrum reuse in the multiple HAP scenario. In the case of many 3G systems the user antenna is either omni-directional or at best low gain, so in these cases it cannot be used to achieve the same effects. The purpose of this chapter is to examine how the unique properties of a WCDMA system can be exploited in multiple HAP uplink architectures to deliver both coverage and capacity enhancement (without the need for the user antenna gain). In addition to the spectral reuse benefits, there are three main benefits for a multiple HAP architecture: • The configuration also provides for incremental roll-out: initially only one HAP needs to be deployed. As more capacity is required, further HAPs can be brought into service, with new users served by the newly deployed HAPs. • Multiple operators can be served from individual HAPs, without the need for complicated coexistence criteria since the individual HAPs could reuse the same spectrum. • HAPs will be payload power, volume and weight constrained, limiting the overall capacity delivered by each platform. Capacity densities can be increased with more HAPs. Moreover, it may be more cost effective 6.1. MULTIPLE HAP SYSTEM SETUP 153 to use more lower capability HAPs [105] (e.g., solar powered planes), rather than one big HAP (e.g., solar powered airship), when covering a large number of cells. The chapter is organized as follows: in section 6.1 the multiple HAP scenario is explained. The interference analysis is presented in section 6.2. In section 6.3 we examine the completely overlapping coverage area case, different numbers of platforms, and simulation results showing the achievable capacity enhancement are presented. Finally, conclusions are presented in section 6.4. 6.1 Multiple HAP system setup In this chapter we use a simple geometric positioning of the high altitude platforms to create signal environments that can easily be compared and analyzed. In each constellation, the HAPs are located with equal separation along a circular contour, as shown in figure 6.1. R qm dm Figure 6.1: An example of a system simulation setup with N = 2 HAPs with overlapping cells of radius R. dm is the distance on the ground between the cell centre and the vertical projection of the HAP on the ground and θm is the elevation angle towards the HAP. The separation distance dm along the line from the vertical projection of the HAP on the ground to the cell centre is varied from 70 km to zero (i.e., all the HAPs will be located on top of each other in the latter case). All HAPs in this chapter are assumed to be flying in the stratosphere at an altitude of 20 km. The size of the coverage area assigned to each HAP is governed by the Chapter 6. Space-Time Processing for Interference 154 Mitigation in HAP WCDMA Systems shape of the base station antenna pattern. If we assume that we only have one cell per HAP, then the coverage area is also synonymous with the total cell area of the HAP. 6.1.1 User Positioning Geometry Each UE (User Equipment) is positioned inside the cell according to an independent uniform random distribution over the cell coverage area with radius R, as shown in figure 6.2. The position of each UE inside each cell is defined relative to the HAP base station that it is connected to, and also relative to every other HAP borne base station. This is necessary in order to evaluate the impact of interference between the different UE-HAP transmission paths. BS 1 BS 2 BS 3 Cell boundary Figure 6.2: A plot showing a sample distribution of 150 UE, where 50 UE are assigned to each of the three base stations (BS1, BS2 and BS3). 6.1.2 Base station antenna pattern The base station antenna pattern for the simulations were chosen to be simple but detailed enough to show the effects of the main and side lobes, especially in 155 6.1. MULTIPLE HAP SYSTEM SETUP the null directions, as illustrated in figure 6.3. A simple rotationally symmetric pattern based on a Bessel function is used for this purpose, and is defined by [1] ⎛ G(ϕ) ≈ 0.7 · ⎝ 2 · J1   ⎞2 sin(ϕ) ⎠ , sin(ϕ) 70π ϕ3dB (6.1) where J1 (·) is a Bessel function of the first kind and order 1, ϕ3dB is the 3 dB beam width in degrees of the main antenna lobe. The 3 dB beam width of the antenna is computed from the desired cell radius according to   cell radius . (6.2) ϕ3dB = 2 · arctan HAP altitude 0 Normalized antenna gain G [dB] ï10 ï20 ï30 ï40 ï50 Cell radius 10 km Cell radius 5 km Cell radius 2 km ï60 ï70 ï100 ï50 0 Eïplane e [degrees] 50 100 Figure 6.3: HAP base station antenna patterns for different cell radii. 6.1.3 User equipment antenna pattern In this analysis we assume that each UE employs a directive antenna and communicates with its corresponding HAP basestation. Using this Chapter 6. Space-Time Processing for Interference 156 Mitigation in HAP WCDMA Systems assumption we only need to set the desired maximum gain of the UE antenna we want to use, as shown Table 6.1. The antenna pattern of the directive antennas is calculated according to 6.1, but with a fixed maximum gain instead of a fixed main beam width, the beamwidth is then ϕ(Gmax ) . User Equipment Mobile phone Data terminal Max. ant. Gain [dBi] 0 2,4,12 Table 6.1: Antenna gains used in the simulation setup. 6.1.4 UE-HAP radio propagation channel model In this chapter we use the Combined Empirical Fading Model (CEFM) together with the Free Space Loss (FSL) model. CEFM combines the results of the Empirical Roadside Shadowing (ERS) model [106] for low elevation angles with the high elevation angle results from [107] for the L and S Bands. Using the FSL model the path loss from UE n to HAP base station m, is given by 2 (4π · dm n) F SL = tx , (6.3) lm,n 2 Gm,n · Grx m,n · λ where dm,n is the line of sight distance between the UE n and HAP m. The rx receiver Grx m,n and transmitter Gm,n antenna gain patterns are calculated using 6.1 and 6.2. The carrier frequency fc used in the simulation is 1.9 GHz which gives a wavelength λ of 0.1579 meters. The CEFM fading loss associated to HAP m is calculated as Lf (θm ) = a · loge (p) + b [dB], (6.4) where p is the percentile outage probability, and the data fitting coefficients a and b are calculated according to [106] 0 2 − 0.15 · θm − 0.7 − 0.2 · fc a = 0.002 · θm , (6.5) b = 27.2 + 1.5 · fc − 0.33 · θm 157 6.1. MULTIPLE HAP SYSTEM SETUP where θm is the elevation angle of HAP m. The total channel gain from UE n to HAP m is then given by   L (θ )  −1 f m F SL 10 . (6.6) gm,n (θm ) = lm,n · 10 6.1.5 WCDMA Setup The different service parameters used in this chapter are collected from the 3GPP standard [108] and are summarized in Table 6.2. In order to account for the relative movement between the UE and the base stations, a fading propagation channel model based on equation 6.6 is simulated. This results in a Block Error Rate (BLER) requirement of 1 % for the 12.2 kbps voice service and a BLER of 10 % for 64, 144 and 384 kbps data packet services, respectively. Parameters Chip rate Data rate Req. Eb /N0 Max. Tx. Power Voice activity Voice 12 kbps 11.9 dB 125 mW 0.67 Type of service Data Data 3.84 Mcps 64 kbps 144 kbps 6.2 dB 5.4 dB 125 mW 125 mW 1 1 Data 384 kbps 5.8 dB 250 mW 1 Table 6.2: WCDMA service parameters employed in the simulation. 6.1.6 Space-Time Processing Techniques The spatial properties of wireless communication channels are extremely important in determining the performance of the systems. Thus, there has been great interest in employing space-time signal processing schemes since they can offer a broad range of ways to improve wireless systems performance. For instance, receiver diversity techniques such as Single-Input MultipleOutput (SIMO) and Multiple-Input Multiple-Output (MIMO) can enhance Chapter 6. Space-Time Processing for Interference 158 Mitigation in HAP WCDMA Systems link quality through diversity gain or increase the potential data rate or capacity through multiplexing gain. In this section, we apply these techniques to HAPs and in the next section we determine their impact on performance via simulations. In this scenario, we assume that the link between the UE and the HAP BS is setup according to the previous sections in this chapter. The total spatio-temporal and polarization degrees of freedom is, in an Orthogonal User Multiple Access SIMO system, restricted by the number of users and the number of receiving antennas. If Es is the average transmit energy per symbol, the received signal r is given by [109]  r = Es · wH hs + wH n, (6.7) where s is the transmitted signal, h is the channel response vector, hn = |hn |ejφn , n = 1, 2, · · · , Nrx , for all receiving antennas, in which |hn | is defined as the inverse of the channel gain in equation 6.6 assuming that the separate channels are independent. The received noise vector n for all receiving antennas is assumed to be AWGN and w are the combining weights at the receiver. Choosing the combining weights w to be equal to the channel response vector h will result in the Maximum Ratio Combining (MRC) method, which can be represented as  (6.8) r = Es · ||h||2 s + hH n. The SNR for the received signal can now be written as 2 √ & % Es · ||h||2 ||h||4 s · Es SNRM RC = = SNRn ·||h||2 = SNRn ·Nrx , = ·E 2 2 2 H σ ||h|| (h n) n (6.9) where SNRn is the signal to noise ratio in each receiving antenna and Nrx is the number of receiving antennas. A similar combining method as in the SIMO receiver diversity is used in the MIMO diversity method. MIMO diversity utilize Ntx transmitting antennas and Nrx receiving antennas and assumes the channel response matrix Hnm = |Hnm |ejφnm , n = 1, 2, · · · , Nrx , m = 1, 2, · · · , Ntx . |Hnm | is the inverse of the channel gain from equation 6.6, and provided that the separate channels are independent then H is a diagonal matrix. The noise is AWGN and the received signal from the MIMO diversity system can then be expressed as [109]  H H Hwtx s + wrx n, (6.10) r = Es · wrx 159 6.2. INTERFERENCE ANALYSIS The SNR for the received signal is then given by 2 √ & % Es · ||H||2F ||H||4F s · Es = SNRn ·Ntx ·Nrx , (6.11) = ·E SNRM RC = 2 σn2 ||H||2F (HH n) where SNRn is the signal to noise ratio in each receiving antenna and Nrx is the number of receiving antennas and Ntx is the number of transmitting antennas. 6.2 Interference analysis Assuming that we have a setup of M different HAPs covering the same cell area and N users connected to each HAP, we can denote each UE position as (xm,n , ym,n ), where n = {1, 2, . . . , N } and m = {1, 2, . . . , M }. An example of a scenario setup with N = 50 and M = 3 is shown in figure 6.2. The maximum power ptx m,n that the user in location (xm,n , ym,n ) is transmitting dependent of the type of service used and can be obtained from Table 6.2. In WCDMA systems, power control is a powerful and essential method exerted in order to mitigate the near-far problem. The power received at base station (HAP) m from user n is tx prx m,n (θm ) = pm,n · gm,n (θm ), (6.12) where gm,n (θm ) is the total link gain, as defined in 6.6, between UE transmitter n and its own cell’s BS receiver m. To be able to maintain a specific quality of service we need to assert that we maintain a good enough SINR (Signal to Interference plus Noise Ratio) level. From Table 6.2 we can see the required Eb /N0 values for different services, and we can express the required SINR, γm,n for user n at HAP base station m as   Eb R req · , (6.13) γm,n = W N0 req where R is the data rate of the service and W is the Chip-rate of the system. The required SINR can then be expressed as req = γm,n prx m,n = M N Itot   m =1 n =1 n =n ptx m,n ptx m,n · pw gm ,n (θm ) + gm,n (θm ) gm,n (θm ) , m = {1, 2, . . . , M } n = {1, 2, . . . , N } (6.14) Chapter 6. Space-Time Processing for Interference 160 Mitigation in HAP WCDMA Systems which can be formulated as γireq = ptx i K  k=1 n =n ptx k , pw gk (θm ) + · gi (θm ) gi (θm ) m = {1, 2, . . . , M } n = {1, 2, . . . , N } i = 1 + (n − 1) + N (m − 1) (6.15) with K = M · N as the total number of users in all cells and pw is the additive req → γireq , gm ,n (θm ) white Gaussian noise (AWGN) at the receiver, γm,n tx tx → gk (θm ), gm,n (θm ) → gi (θm ), pm ,n → pk are performed according to the index mapping rules in equation (6.15). To solve for the transmitter power ptx k of each of the K individual UE simultaneously 6.14 can be reformulated into a matrix form (see appendix C) as ptx = (I − A) −1 b, (6.16) where the calculated vector ptx contains the necessary transmitter power level assigned to each of the K UE to fulfil the SINR requirement and where matrix [A]K×K and vector [b]K×1 are defined as [aik ]K×K = γireq · gk (θm ) gi (θm ) pw , gi (θm ) n = {1, 2, . . . , N } , i = 1 + (n − 1) + N (m − 1) [aik ] = 0 for n = n, m = {1, 2, . . . , M } , m = {1, 2, . . . , M } , for n = n and [bi ]K×1 = γireq · n = {1, 2, . . . , N } , k = 1 + (n − 1) + N (m − 1) (6.17) Using the prx = g  ptx , where  denotes an elementwise multiplication and g is the total channel gain vector [gk ]K×1 for all k = {1, 2, . . . , K} users, then all elements in the vector prx for each block that contain the UE of each of the M cells are balanced. The total cell interference can then be calculated as N  own prx m = {1, 2, . . . , M } (6.18) Im (θm ) = m,n (θm ), n=1 oth (θm ) = Im M  N  m =1  m =m n=1 prx m ,n (θm ) + pw , m = {1, 2, . . . , M } (6.19) 6.3. SIMULATION RESULTS 161 own where pw is the thermal noise at the receiver, Im (θm ) is the interference oth from the UE within the own cell m and Im (θm ) is the interference from the UE in the M − 1 other cells where M is the total number of cells. We can now calculate iU L (θm ) which defines the other to own interference ratio for the uplink to HAP m and is given by iU L (θm ) = oth Im (θm ) . own Im (θm ) (6.20) This is a performance measure of the simulated system capacity at a specific elevation angle θm towards the HAP (see figure 6.1). If iU L (θm ) is between zero and one there is possibility to have multiple HAP base stations covering the same coverage area. The actual number of users that can access the HAP base stations is also dependent of which data rate each user is using for transmission. 6.3 Simulation Results In this simulation we assume M HAPs uniformly located along a circular boundary, with the centre of the circular boundary acting as the pointing direction of the HAPs base station antennas which simulate several overlapping cells, see figure 6.1. The beamwidth of these base station antennas are determined by the radius of the cell coverage area (see figures 6.1 and 6.3). These results are acquired through running Monte Carlo simulations of the multiple HAP system. The aim of the simulation is to assess the effect of adding more HAPs on the system’s capacity and of the impact of using spacetime diversity techniques. The distance dm between the cell centre and the vertical projection of the HAP on the earth’s surface is denoted as ”distance on the ground” and is varied from 0 to 70 km with a fixed cell position, as shown in figure 6.4. The distance to the cell centre is also changing the elevation angle θm towards the HAP base station m as seen from the user. The cell radius has been set to 10 km and 30 km, and the HAP altitude is 20 km. Each HAP base station serves 100 users within each corresponding cell. From figure 6.5 it is clear that with the smaller cell radius (10 km) the worst case scenario will occur when all the HAPs are stacked on top of each other at 90 degrees elevation angle from the cell centre (i.e., at a distance dm on the ground of 0 km). In the larger cell radius case (30 m) the worst case scenario happens approximately at 30 km which is at the edge of the cell. Chapter 6. Space-Time Processing for Interference 162 Mitigation in HAP WCDMA Systems R qm dm Figure 6.4: A plot illustrating the change of HAP position dm to create different elevation angles θm . Comparing the bottom diagram in figure 6.5 with the two diagrams in figure 6.6, we can see that if we utilize a maximum allowed other-to-own interference ratio equal to one, then as the service data rate decreases, the number of possible HAP base stations covering the same area can increase from 2-4 HAPs (depending on the distance dm between the cell centre and the vertical projection of the HAP on the ground) for the combined service (12 kbps and 384 kbps) to 6 HAPs with the same service (12 kbps on all HAPs). Next, we analyze the impact of different space-time diversity techniques (SIMO and MIMO) on the possible number of HAPs that can coexist within the same cell area and compare them to a single-input single-output (SISO) system. From figure 6.7 it is obvious that using a space-time diversity technique will enhance the interference mitigating capability and improve the overall performance of the multiple HAP system. This interference mitigation technique can also be interpreted as a capacity improvement, which is clearly seen in figure 6.7 for a three HAP system and in figure 6.8 for a seven HAP system. In both of these figures we can observe a decrease in the other-toown interference ratio as we use an increasing number of antennas at the transmitter and receiver, which in turn will allow more HAPs to provide wireless service to more users by utilizing the remaining degrees of freedom of the system. Comparing the graphs in figure 6.8, we can observe that a seven HAP 6.3. SIMULATION RESULTS 163 Figure 6.5: The performance of the voice service (12 kbps) from one HAP in combination with the data service (384 kbps) on the remaining HAPs for cell radius of 10 km (top) and 30 km (bottom). The distance on the ground dm is varied from 0 to 70 km. Chapter 6. Space-Time Processing for Interference 164 Mitigation in HAP WCDMA Systems 1.1 5 HAPs 4 HAPs 3 HAPs 2 HAPs Other to Own interference ratio iul 1 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 0.1 0 10 20 30 40 50 Distance on the ground [km] 60 70 1.4 6 HAPs 5 HAPs 4 HAPs 3 HAPs 2 HAPs 7 HAPs Other to Own interference ratio iul 1.2 1 0.8 0.6 0.4 0.2 0 0 10 20 30 40 50 Distance on the ground [km] 60 70 Figure 6.6: The other to own interference ratio obtained for a 30 km cell radius for: (top) the performance of the voice service (12 kbps) from one HAP in combination with the data service (144 kbps) on the remaining HAPs and (bottom) the performance when we have voice services (12 kbps) on all HAPs. The distance on the ground dm is varied from 0 to 70 km. 165 6.3. SIMULATION RESULTS 1 SISO 1x2 SIMO 1x4 SIMO 2x2 MIMO 2x4 MIMO 4x4 MIMO 8x8 MIMO Other to own interference ratio iUL 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 0.1 0 0 10 20 30 40 50 60 Distance on the ground dm [km] 70 80 Figure 6.7: The other to own interference ratio obtained for a 30 km cell radius for: the performance of the voice service (12 kbps) from one HAP in combination with the data service (384 kbps) on the remaining two HAPs and utilizing different SISO, SIMO and MIMO space-time diversity systems. The distance on the ground dm is varied from 0 to 70 km. Chapter 6. Space-Time Processing for Interference 166 Mitigation in HAP WCDMA Systems SISO 1x2 SIMO 2x2 MIMO 4x4 MIMO 8x8 MIMO Other to own interference ratio i UL 1.5 1 0.5 0 0 10 20 30 40 50 60 Distance on the ground d [km] 70 80 m Figure 6.8: The other to own interference ratio obtained for a 30 km cell radius for: the performance of the voice service (12 kbps) from one HAP in combination with the data service (384 kbps) on the remaining six HAPs and utilizing different SISO, SIMO and MIMO space-time diversity systems. The distance on the ground dm is varied from 0 to 70 km. 6.4. CONCLUSIONS 167 system using SISO would not be possible due to the interference. However, a SIMO diversity system (utilizing two receiving antennas at the HAP base station) would make a seven HAP system possible. Adding more antennas at the receiver and transmitter respectively will increase the number of possible HAPs that can be used in the multiple HAP system. However, the benefit of the diversity system will diminish even with increasing the number of antennas beyond a certain limit. From figure 6.7 and figure 6.8 it is obvious that this limit is obtained at approximately a 4x4 MIMO system, beyond which diversity gain is negligible as is evident from the graph of the MIMO 8x8 system. It is also clear from figure 6.6 that the worst case distance (highest interference level) is at approximately 30 km, and consequently a worst case elevation angle of 34 degrees. This maximum interference level depends on the cell radius chosen for the HAP base station as shown in figure 6.9. Simulation results show that for cell radii larger than 10 km the maximum interference level will occur at the cell boundary. 6.4 Conclusions In this chapter we have investigated the possibility of multiple HAP coverage of a common cell area in WCDMA systems with and without space-time diversity techniques and in particular we have studied the uplink. From these simulations it is shown that as the service data rate decreases, the number of possible HAP base stations that can be deployed to cover the same geographical area increases. It has further been shown that this increment in number of HAP base stations can be enhanced to some extent by using spacetime diversity techniques. We have also shown that the worst case position of the HAPs is in the centre of the cell if the cell radius is small (≤ 20 km) and at the cell boundary for large cells (≥ 20 km). We can conclude that there is a possibility of deploying 3-5 (SISO), or 5-8 (1x2 SIMO, 2x2 MIMO and 4x4 MIMO) HAPs covering the same cell area in response to an increase in traffic demands, depending on the type of service used. There also appear to be a limit on the number of HAPs that could be deployed using spacetime diversity techniques. Simulation results have shown that the maximum number of HAPs that could be sustained is approximately eight when using the voice services with 4x4 MIMO on all HAPs and users. Chapter 6. Space-Time Processing for Interference 168 Mitigation in HAP WCDMA Systems 1 50 km 30 km 20 km 10 km 5 km Other to Own interference ratio iul 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 0.1 0 0 10 20 30 40 50 Distance on the ground [km] 60 70 80 Figure 6.9: Illustrating the effect of HAP base station cell radius on interference levels. A system of 3 HAPs is utilized here and a voice service (12 kbps) from one HAP in combination with the data service (384 kbps) on the other HAPs. The distance on the ground dm is varied from 0 to 70 km. CHAPTER 7 COOPERATIVE SPACE-TIME PROCESSING FOR POWER EFFICIENT WIRELESS SENSOR NETWORKS W ireless Sensor Networks (WSN) have been attracting great attention recently. They are relatively low cost to be deployed and to be used in many promising applications, such as biomedical sensor monitoring (e.g., cardiac patient monitoring), habitat monitoring (e.g., animal tracking), weather monitoring (temperature, humidity, etc.), low-performance seismic sensing, environment preservation and natural disaster detection and monitoring (e.g., flooding and fire) [114–118]. The WSN applications analyzed in this chapter have a topology where a large number of wireless sensor nodes are spread out over a large or small geographic area (e.g., disaster regions, indoor factory, large sports event areas, etc.). In this topology, an inefficient use of bandwidth and transmitter power resources is resulted if each wireless sensor is transmitting its measurement data to the base station (processing central). In this case, each sensor node would have to be assigned its own frequency channel and, if the base station is located a long distance from the sensor nodes, it would also demand a higher than average sensor node transmitter power. By using a coordinating cluster head, for each cluster of wireless sensor nodes, we can instead use the combined transmitter power of the node cluster through the use of beamforming to increase the transmitter-receiver separation and/or to improve the signal-to-noise ratio (SNR) of the communication link. Another Chapter 7. Cooperative Space-Time Processing for 170 Power Efficient Wireless Sensor Networks advantage of using this cooperative transmission is that we can exert power control to minimize the power consumption of each individual sensor node, and thus maximizing network lifetime. In addition, in a cooperative network the measurement data could be sent by using Time Division Multiplexing (TDM) instead of Frequency Division Multiplexing (FDM) which improves the overall bandwidth efficiency of the system. In this chapter, we propose to use a cooperative beamforming approach in wireless sensor networks to increase the transmission range, minimize power consumption and maximize network lifetime. This will be of particular interest for outdoor applications, especially when monitoring remote areas using aerial vehicles such as a High Altitude Platform (HAP) or Unmanned Aerial Vehicle (UAV) as a platform for the data collecting base station. We will investigate how the required transmitter power of each sensor node is affected by the number of cooperating transmission nodes in the network. In addition, we will also study if mitigation of fixed interference can be achieved in this type of random antenna array by exploiting ”null” directions in the beamforming pattern. Finally, we present a comparison in the use of beamforming with the different forms of diversity systems such as Multiple-Input Single-Output (MISO), SingleInput Multiple-Output (SIMO) and Multiple-Input Multiple-Output (MIMO) for the same purpose of achieving a longer transmission distance (or range) while maintaining a low energy consumption. Beamforming can of course be interpreted as a form of MISO system although it differs from the normal view of how a diversity system operates. This chapter is organized as follows: Section 7.1 presents an overview and analysis of cooperative beamforming using a large aperture random array. In section 7.2 is given a brief description of MISO, SIMO and MIMO diversity schemes and analysis using the Rice distributed fading channel model employed in the simulation. Section 7.3 present the numerical results of the simulated beamformer and MISO, SIMO and MIMO diversity systems. Finally, section 7.4 list the concluding remarks. 7.1 Cooperative Beamforming In this chapter we use the delay-and-sum beamforming technique which is the oldest and simplest algorithm for Space-Time processing. This beamforming is done through coherent excitation/reception of amplitude and phase of the signal transmitted/received from each individual antenna element in a collection or cluster of similar antenna elements also known as an antenna array [119]. Antenna arrays can have different configurations (e.g. linear, 7.1. COOPERATIVE BEAMFORMING 171 planar, circular, triangular, rectangular or spherical etc.). Extensive research has been done on uniform array beamforming using one (linear) or two (planar) dimensional equi-distant element arrays [119–121]. In addition, there is also work done on beamforming using circular, triangular and rectangular arrays [1, 119]. The antenna array formed by the individual sensor node antennas is assumed to be a planar array, of randomly positioned sensor node antennas, which is parallel with the plane containing all sensor nodes so that the sensor nodes are only extended in x and y direction and not in z direction. This is a valid assumption in most cases since the elongation of the networks in z direction in most cases is very small compared to the distance between the network cluster and the base station we want to communicate with [124]. The design of this type of cooperative array is similar to the design of large aperture arrays where we have an inter-element spacing that is random and larger than half the wavelength. There are no known simplifying techniques for synthesis of randomly spaced arrays, like Schelkunoffs polynomial method [1, 119] or the Fourier Transform method [1, 119]. In the random array all properties e.g array pattern, beam width, sidelobe level and gain are stochastic variables. In figure 7.1 we show a scenario with N = 50 sensor nodes deployed inside a circular boundary in the x-y plane with the radius R. The distribution of these sensor nodes is uniform and independent. The nth sensor then has the polar coordinates (rn , φn ) . The signal yn (t) at the array sensor node n can then be expressed as yn (t) = s(t − α0 · x0 ), (7.1) where s(t) is the signal to be transmitted/received and the nth sensor at location xn transmits/receives the electromagnetic signal yn (t). The slowness vector α0 is the required delay for each sensor to steer the array in a specific direction toward the signal source or target, and is defined as α0 = d0 c (7.2) where d0 is the direction of the wave propagation and c is the speed of light. The total output of the delay-and-sum algorithm can be expressed by z(t) = N −1  n=0 α − α0 )·x0 ), wn s(t + (α (7.3) Chapter 7. Cooperative Space-Time Processing for 172 Power Efficient Wireless Sensor Networks R Figure 7.1: 50 sensor nodes positioned according to an independent uniform distribution within a cluster area of radius R. 7.2. SPATIAL DIVERSITY TECHNIQUES 173 where wn is the amplitude weights of the array tapering and α is the slowness vector for the direction of observation. If we assume that all the sensor nodes are approximately located in the same plane (i.e. the x-y plane) and the source/target is located at the spherical coordinates d0 = (d0 , φ0 , θ0 ) in the far-field, and we are transmitting a narrow band signal then we can approximate (7.3) as (see appendix D) G(φ, θ) = N −1 rn 1  wn ejω(t− c (cos(φn )u+sin(φn )v) , N n=0 (7.4) where u = sin(θ) cos(φ)−sin(θ0 ) cos(φ0 ) and v = sin(θ) sin(φ)−sin(θ0 ) sin(φ0 ) for the direction of the incoming/outgoing wave (φ0 , θ0 ) and the direction of observation (φ, θ). The function G(φ, θ) is then one ensemble of the array amplitude gain function for one set of stochastic sensor locations. To find the ensemble mean of the array amplitude gain functions we assume an independent uniform distribution of the sensor locations within the radius R,  (7.5) E{G(φ, θ)} = G(φ, θ)pR,φ (rn , φn ), where pR,φ (rn , φn ) is the probability density function (PDF) of the sensor locations. In figure 7.2 we show the absolute squared average array gain function |E{G(φ, θ)}|2 of 250 realizations of the array amplitude gain function G(φ, θ), and in figure 7.3 we show the standard deviation for the distribution of the amplitude sidelobe levels. From figure 7.2 we can also estimate a mean sidelobe level that will converge toward ≈ −17 dB which is consistent with the theoretical value, N −1 . The average signal to noise ratio of the array is defined as SN Rarray = SN Rnode · G(φ, θ) which means that the array average SNR is SN Rarray = N · SN Rnode when we are aiming the array toward the incoming assumed plane wave. The SN Rarray is a Gaussian distributed parameter with a mean of 17 dB, and a 95% confidence that the SNR of the array will be higher than 7 dB. 7.2 Spatial Diversity Techniques Another recently popular technique to improve the signal to noise ratio of the long range transmission is to use some form of spatial diversity technique like Multiple-Input Single-Output (MISO), Single-Input Multiple-Output (SIMO) Chapter 7. Cooperative Space-Time Processing for 174 Power Efficient Wireless Sensor Networks Figure 7.2: A plot showing a small part around the main lobe of the absolute squared average array pattern of 250 realizations of the random sensor locations. Normalized Array Gain G 0.8 0.6 + Standard deviation Mean Gain 0.4 0.2 0 ï0.2 ï0.4 170 ï Standard deviation 175 180 185 Array aiming direction q0 [deg] 190 Figure 7.3: A cross-section of the main lobe of all 250 realizations of the array amplitude gain pattern. 7.2. SPATIAL DIVERSITY TECHNIQUES 175 or Multiple-Input Multiple-Output (MIMO) antenna system. In the following analysis of these diversity techniques we are assuming a perfect knowledge of the propagation channel. 7.2.1 Cooperative MISO and SIMO Consider a frequency flat fading propagation model with Ntx antenna elements at the transmitter and one antenna element at the receiver. To take full advantage of the antenna transmit diversity we send multiple weighed copies of the signal sample through all the transmitting antenna elements. The received baseband signal sample can then be expressed as + r[m] = L−1 Es  hl wl s[m] + n[m], Ntx (7.6) l=0 where r[m] ∈ C is the received sample, s[m] ∈ C is the transmitted sample and n[m] is a noise sample with n[m] ∼ CN (0, σn2 ). The coefficient wl is the channel weight for channel l and Es is the transmitted average symbol energy. This can be expressed in vector notation as + Es hws + n, (7.7) r= Ntx where h ∈ CNtx ×1 is the frequency flat fading channel vector with a Rice distribution. The normalized Rician channel vector h can then be defined as [125] √ √ (7.8) h  c1 l + c2 Rtx hn , where l is the line of sight (LOS) component represented as a mean value that satisfies the condition |l|2 = Ntx , and Rtx is the transmit correlation vector. Rtx is assumed to be positive definite full rank matrix. hn ∼ CN Ntx (0Ntx , 1Ntx ) is a complex valued Gaussian vector representing the non line of sight (NLOS) component. The coefficients c1 = K/(K + 1) and c2 = 1/(K + 1) are normalizing factors, where K is the Rice factor which represents the power ratio between the LOS and NLOS components. The weight vector w that maximizes the received SNR is given by w=  hH , Ntx h (7.9) Chapter 7. Cooperative Space-Time Processing for 176 Power Efficient Wireless Sensor Networks which is the transmit maximum ratio combining (MRC) method and is also known as matched beamforming. The SNR of the received signal can then be expressed as γrx = Es · |h|2 . N0 (7.10) The second type of spatial diversity is receive diversity in which we are utilizing a single input multiple output (SIMO) frequency flat fading propagation channel model with Nrx receiving antenna elements and a single transmitting antenna element. To fully exploit the receive diversity we will receive multiple copies of the transmitted signal through all the Nrx receiving antenna elements. The received baseband signal sample can then be expressed as + L L  Es  (wl hl )s[m] + wl nl [m], (7.11) r[m] = Nrx l=1 l=1 where rl [m] ∈ C is the received sample from receiving antenna element l , s[m] ∈ C is the transmitted sample and nl [m] is a noise sample at receiving antenna element l with nl [m] ∼ CN (0, σn2 ). the coefficient wl is the channel weight at receiving antenna element l and Es is the transmitted average symbol energy. This can be expressed in vector notation as  (7.12) r = Es wH hs + wH n, where h ∈ CNtx ×1 is the frequency flat fading channel vector with a Rice distribution. The normalized channel vector h can then be defined as [125] h √ c1 l + √ c2 Rrx hn , (7.13) where l is the line of sight (LOS) component represented as a mean value that satisfies the condition |l|2 = Nrx , and Rrx is the receive correlation vector. Rrx is assumed to be a positive definite full rank matrix. hn ∼ CN Nrx (0Nrx , 1Nrx ) is a complex valued Gaussian vector representing the non line of sight (NLOS) component. The weight vector w that maximize the received SNR at each antenna element is given by w=  Nrx hH . h (7.14) 7.2. SPATIAL DIVERSITY TECHNIQUES 177 The SNR of the received signal after we have performed a maximum ratio combining (MRC) can then be expressed as γrx = 7.2.2 Es · |h|2 . N0 (7.15) Cooperative MIMO By combining the MISO and SIMO diversity techniques we create a system of (Ntx and Nrx ) transmitting and receiving antenna elements respectively. If we consider a frequency flat fading (Ntx × Nrx ) MIMO propagation model the received signal can be written in vector notation as + Es H w Hwtx s + wrx n. (7.16) r= Ntx rx In the MIMO case the Rice distributed channel matrix H can be derived as H 1 1 √ √ 2 2 c1 L + c2 Rrx Hn Rtx , (7.17) where L represents the LOS component and is the arbitrary rank mean value matrix with the condition that Tr(LLH ) = Nrx · Ntx , Rrx and Rtx are the correlation matrices on the transmitter and receiver side respectively. Hn ∼ CN Nrx ,Ntx (0Nrx ×Ntx , INrx ⊗ INrx ). To maximize the combined SNR at the receiver antenna elements we maximize 1 H 12 Hwtx 1 Es 1wrx · . (7.18) γrx = N0 Ntx wrx 2 γrx is then maximized when wrx and wtx /Ntx are equal to the singular input and output vectors of the channel matrix H corresponding to the maximum singular value of the channel matrix H. Equation 7.16 can then be written as  (7.19) r[m] = Es σmax s[m] + n[m]. where σmax is the maximum singular value of the channel matrix H and since 2 is the same as the maximum eigenvalue λmax of HHH we can now σmax express the received SNR of the MIMO diversity technique as γrx = Es · λmax . N0 (7.20) Chapter 7. Cooperative Space-Time Processing for 178 7.3 Power Efficient Wireless Sensor Networks Simulation Results If we consider a base station mounted on an aerial platform such as a HAP or a UAV to collect data from remote sensor networks then the amount of obstructions in the transmission path would depend on the type of environment at the sensor locations, although it can still generally be assumed that the number of obstructions will increase with a decreasing antenna elevation angle. Therefore the propagation effect of the change in elevation can be translated into a change of the Rice distribution K-factor. In the presented simulations, the Rician K-factor was varied over an  interval of K ∈ 1 · 10−8 , 1 · 10+8 , where the low value represents a channel with no LOS component and very little correlation between the different signal paths and therefore resembles a Rayleigh fading channel. When the Rician K-factor is gradually increased the correlation between the signal paths will increase and the Direction of Departure/Direction of Arrival of the signals will narrow into a smaller and smaller angular sector, until the K-factor asymptotically goes toward infinity and all signal paths will be correlated and pointing in the same direction. In figure 7.4 we see the comparison between the ordinary random array beamformer performance and the MISO/SIMO diversity systems performance. Inspecting figure 7.4, we can see that the MISO/SIMO diversity system seems to maintain a constant low node transmitter power Ptx even in a NLOS scenario by spreading the energy over multiple paths instead of transmitting it all in one direction. Furthermore, we can see from figure 7.4 that if the distance between the transmitting nodes and the basestation is increased from 1 km to 10 km, the nodes need a 100 fold increase of the total transmitted power to maintain the same capacity. This is independent of whether we are using the nodes as a beamforming array or a diversity system, which is consistent with the inverse square law of the free space loss. If we now increase the number of receiving antenna nodes to be equal to the number of transmitting antenna nodes we get a 50 × 50 MIMO system which will increase the array and diversity gains even further. This effect can clearly be seen in figure 7.5 where the performance of the MIMO system outperforms the other systems in both LOS and NLOS scenarios. 179 7.3. SIMULATION RESULTS 4 10 Required node transmitter power Ptx [W] Array ï Node Ptx at 10 km receiver distance Array ï Node Ptx at 1 km receiver distance 2 10 MISO ï Node Ptx at 10 km receiver distance MISO ï Node Ptx at 1 km receiver distance 0 10 ï2 10 ï4 10 ï6 10 ï8 10 ï80 ï60 ï40 ï20 0 20 40 Riceïfactor 10 u log10 ( K ) [dB] 60 80 Figure 7.4: Comparison between of the Array Beamformer and MISO/SIMO system for different K-factor values at two different distances from the base station of 10 km and 1 km, respectively. 8 10 Required node transmitter power Ptx [W] SISO ï Node Ptx Array ï Node Ptx 6 10 MISO/SIMO ï Node Ptx MIMO ï Node Ptx 4 10 2 10 0 10 ï2 10 ï4 10 ï80 ï60 ï40 ï20 0 20 40 Riceïfactor 10 u log10 ( K ) [dB] 60 80 Figure 7.5: Performance of the Array Beamformer, MISO/SIMO and MIMO systems for different K-factor values and compared with a single antenna SISO system. Chapter 7. Cooperative Space-Time Processing for 180 7.4 Power Efficient Wireless Sensor Networks Conclusions In this chapter we have investigated how the required transmitter power of each sensor node is affected by the number of cooperating transmission nodes in a traditional random beamformer array. Due to the randomness of the sensor node positions there is no simple algorithm for mitigation of interference from a fixed direction. This is because the sidelobe levels and the sidelobe positions are random. A comparison in the use of beamforming with diversity systems such as MISO/SIMO and MIMO for the same purpose of achieving a longer transmission distance or maintaining a low energy consumption. It is clear from these investigations that the MISO/SIMO and MIMO diversity systems are superior in performance to both the SISO link and the traditional form of array beamforming, especially when the LOS component is small or non-existent. The best performance though, is given by the MIMO system where we have multiple antenna nodes on both the transmitting and receiving end of the link. Even one extra antenna at the receiving basestation will increase the performance of the system two-fold in a LOS scenario and give an improved performance in NLOS as well. CHAPTER 8 CONCLUSIONS T his thesis has presented an extended scope of space-time processing by proposing novel applications in a variety of wireless communication systems. These have included increasing the spectral efficiency of satellite and high altitude platform (HAP) communication systems, enhancing link quality for Bluetooth links in indoor office environments, reduction of possibly harmful electromagnetic radiation from mobile phones, enhancing the coverage and capacity of integrated multiple-HAP 3G systems, and improving the energy efficiency of cooperative wireless sensor networks (WSN). • In chapter 2 we proposed a novel multiple antenna channel model and associated simulator which takes into account the spatial, temporal and polarization (STP) properties affecting signal transmission in wireless communications. In addition, we presented the theoretical background and analysis, features and properties, and implementation of the proposed STP channel simulator. Further, we tested the simulator for various propagation conditions. The results of the simulator have shown good agreement with the theoretical ones. We have also investigated the impact of depolarization on the probability distributions of the simulated signals and their adverse effect on performance. The proposed STP simulator was employed in chapter 3 to investigate the performance of satellite and high altitude platform communication links. • In chapter 3 we investigated the potential gain of using a MIMOOFDM antenna system in combination with platform diversity in 182 Chapter 8. Conclusions order to increase the capacity of satellite and high altitude platform communication systems. Simulation results have shown that the platform diversity system provides superior performance as compared to the single platform system and that by careful design of the 3D MIMO antenna array we can create independent space-polarization sub-channels for increasing the capacity through multiplexing. In addition, a novel multi channel fading simulator which takes into account the temporal, spatial and polarization properties experienced by these systems was developed and tested in different propagation scenarios. • Chapter 4 investigated the wave propagation effects of a short-range wireless device, such as the Bluetooth technology. Specifically, we assessed the fading phenomenon for Bluetooth link in an indoor office environment by simulation of different propagation scenarios and used measurement results to confirm our findings. The investigations were carried out using FEM to model the electromagnetic wave propagation for NLOS and LOS propagation scenarios. The measurement trails and simulations were shown to be in good agreement. This was also confirmed by comparison with the theoretical statistical probability distribution of the signal in both scenarios. A power-distance exponential propagation law was found to be sufficient to describe the propagation for corridors (where a wave guide phenomena was observed) and through office walls. In addition, we investigated a diversity system utilizing different combining techniques in spatial diversity and spatial multiplexing schemes, and assessed their performance over a fading radio channel in a NLOS propagation environment. Our results show a substantial gain is achieved by using a MIMO spatial multiplexing system. • In chapter 5 we presented a FEM model which simulate a physical MIMO antenna system which is controlled by various adaptive signal processing algorithms in order to suppress the electromagnetic field at a certain volume in space. We have also presented the solution for constraining the total output power of the system to a predefined level. Further, we have investigated the effects of the size and number of MIMO antenna elements on the performance of the system and also tested the algorithms at different carrier frequencies. The SAR attenuation levels achieved from these simulations suggest the possibility of using an active antenna system for the reduction of electromagnetic field density. However, our result also show some limitations associated 183 with implementing these antenna arrays in mobile phones, for which further research is needed to find practical solutions. • In chapter 6, we investigated the possibility of multiple HAP coverage of a common cell area in WCDMA systems with and without space-time diversity techniques and in particular we have studied the uplink. From the simulations we have shown that as the service data rate decreases, the number of possible HAP base stations that can be deployed to cover the same geographical area increases. It has further been shown that this increment in number of HAP base stations can be enhanced by using space-time diversity techniques. It was also concluded that there is a possibility of deploying 3-5 (SISO), or 5-8 (1x2 SIMO, 2x2 MIMO and 4x4 MIMO) HAPs covering the same cell area in response to increase traffic demands, depending on the type of service used. Simulation results have also shown the limit on the number of HAPs that could be deployed using space-time diversity techniques. • Finally, in chapter 7 we have investigated how the required transmitter power of each sensor node in a WSN could be improved upon by using cooperating transmission nodes either as a traditional random beamformer array or as a diversity system. A comparison between the diversity systems (MISO, SIMO and MIMO) with the beamformer for the purpose of achieving a longer transmission distance or maintaining a low energy consumption was performed. Simulation results have shown that the diversity systems are superior in performance to both the SISO link and the traditional form of array beamforming. This thesis has clearly shown the varied applications of space-time processing in wireless communication systems, and the broad range of ways they play in improving the performance and economics of these systems. This is the reason why space-time processing is seen as one of the main critical components in future wireless communication systems. Consequently, further research into these applications and other applications is still necessary in order to optimize energy efficiency, capacity, coverage and quality of these systems. 184 Chapter 8. Conclusions APPENDIX A SPHERICAL VECTOR HARMONICS APPENDIX A.1 187 Spherical Vector Harmonics The spherical vector harmonics are defined for l > 0 as: ⎧ ⎪  lm (θ, φ)  lm (θ, φ) =  1 ⎪ LY (TE-multipole) ⎪X ⎨ l(l + 1) 1 ⎪ ⎪X ˆ  lm (θ, φ) (TM-multipole)  ⎪ LY ⎩ lm (θ, φ) = r ×  l(l + 1) (A.1)  = −jr×∇ is an angular momentum operator borrowed from quantum where L physics. Ylm is the scalar spherical harmonics and is a function of the angular spherical coordinates θ and φ. 1 Plm (cos θ)ejmφ Ylm (θ, φ) = √ 2π (A.2) where Plm is the associated Legendre function of the first kind, degree l, order 1 m and normalized to unity −1 (Plm (x))2 dx = 1. Plm (cos θ) = sinm θ dm Pl (cos θ) d(cos θ)m (A.3) where Pl is the Legendre polynom. The vector spherical harmonics form a complete orthonormal set for tangent vector fields on the spherical surface. This describes the tangential behavior of the solution of Helmholtz equation obtained by separation of variables in a spherical coordinate system. ⎧  lm (θ, φ) (TE-modes) ⎨ η0 gl (kr)X (A.4) ⎩ jη0 ∇ × fl (kr)X  lm (θ, φ) (TM-modes) k where k is the wave number, fl (kr) and gl (kr) are spherical Hankel functions fl = jl ± jyl with jl being the spherical Bessel function and yl the spherical Neuman function. A vector field satisfying the homogenous vector Helmholtz equation in a spherical shell can be written as a weighted sum of the TE and TM modes ( 'j  lm ) + aM (l, m)gl (kr)X  lm  = η0 aE (l, m)(∇ × fl (kr)X (A.5) E k l,m 188 A.1. SPHERICAL VECTOR HARMONICS A similar derivation can be formed for the magnetic vector field. The weights aE (l, m) for the electric multipole moments and aM (l, m) for the magnetic multipole moments can be evaluated by making use of the orthogonality property of the spherical harmonics [2, 3]  ∗ ·E  dΩ (A.6) aE (l, m)jl (kr) = X lm where we get the electric multipole weight aE (l, m) by projecting the electric far-field of the antenna on to the vector spherical harmonics. This results  lm is for a in the weight aE (l, m) expressing how strong a certain mode X particular antenna far-field pattern. The magnetic multipole weight aM (l, m) is derived in a similar manner. For simplicity we are using an asymptotic far-field approximation of these multipole weights [2, 3]. ⎧  1 k ⎪ ∗  dΩ ⎪  Ylm (l, m)f (kr) ≈ · (θ, φ) r · E a ⎪ E l ⎨ η0 l(l + 1)  (A.7) k ⎪ ∗ ⎪  ⎪ Ylm (θ, φ) r · H dΩ ⎩ aM (l, m)gl (kr) ≈ −  l(l + 1) APPENDIX B ANTENNA TYPES APPENDIX B.1 Antenna types Figure B.1: Antenna type: Half wave model 1 Figure B.2: Antenna type: Half wave model 2 Figure B.3: Antenna type: Half wave model 3 191 192 B.1. ANTENNA TYPES Figure B.4: Antenna type: Quarter wave model 2 Figure B.5: Antenna type: Quarter wave model 1 APPENDIX C WCDMA POWER CONTROL 195 APPENDIX C.1 WCDMA Power Control Derivation of Equation (6.16): Equation (6.14) can be reformulated by multiplying with the expression of the total interference on both sides of the equation ⎡ ⎤ γireq K ⎢ pw ⎥ gk (θm ) ⎢ ⎥ = ptx + ptx k · i . ⎣ gi (θm ) gi (θm ) ⎦ (C.1) k=1 n =n Multiplying each term inside the brackets with γireq will then yield K  γireq · k=1 n =n gk (θm ) tx pw · pk + γireq · . gi (θm ) gi (θm ) (C.2) Substituting each term with an indexed variable according to gk (θm ) gi (θm ) pw req , = γi · gi (θm ) [aik ]K×K = γireq · [bi ]K×1 for n = n and, [aik ] = 0 for n = n (C.3) will simplify Equation (C.2) into K  tx ai,k · ptx k + bi = p i , (C.4) k=1 n =n By identifying K k=1 n =n ai,k · ptx k as a matrix multiplication we can now write Equation (C.4) in matrix form as A · ptx + b = Iptx . (C.5) Rearranging Equation (C.5) we now solve for the necessary transmitter power ptx to fulfil the required SINR for a particular quality of service. ptx = (I − A) −1 b (C.6) 196 C.1. WCDMA POWER CONTROL APPENDIX D BEAMFORMING APPENDIX D.1 199 Beamforming Derivation of Equation (7.3): The slowness vector α in (7.2) is defined as α= d . c (D.1) The d vector represents the direction of observation and can be expressed in cartesian coordinates as d = d · {− sin(θ) cos(ϕ), − sin(θ) sin(ϕ), cos(θ)} . (D.2) Assuming that the sensor nodes are only distributed in the x − y plane. 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Collings, Improved General Lower Bound for Spatially-Correlated Rician MIMO Capacity, IEEE Communications Letters, Vol. 10, No. 3, March 2006. Wireless mobile communication networks are rapidly growing at an incredible rate around the world and a number of improved and emerging technologies are seen to be critical to the improved economics and performance of these networks. The technical revolution and continuing growth of mobile radio communication systems has been made possible by extraordinary advances in the related fields of digital computing, highspeed circuit technology, the Internet and, of course, digital signal processing. Improved third generation (3G) and future generation wireless communication systems must support a substantially wider and enhanced range of services with respect to those supported by second generation and basic 3G systems. The never-ending quest for such personal and multimedia services, however, demands technologies operating at higher data rates and broader bandwidths. This combined with the unpredictability and randomness of the mobile propagation channel has created many new technically challenging problems for which innovative, adaptive and advanced signal processing techniques may offer new and better solutions. Space-time processing techniques have emerged as one of the most promising areas of research and development in wireless communications for the efficient utilization of the physical mobile radio propagation channel. Space-time processing signifies the signal processing performed on a system consisting of several antenna elements, whose signals are processed adaptively in order to exploit both the spatial (space) and temporal (time) dimensions of the radio channel. This can significantly improve the capacity, coverage, quality and energy efficiency of wireless systems. This thesis expands the scope of space-time processing by proposing novel applications in wireless communication systems. These include the reduction of possibly harmful electromagnetic radiation from mobile phones, enhancing the quality of Bluetooth links in indoor office environments, increasing the spectral efficiency of satellite and the novel high altitude platforms (HAPs) communication systems, enhancing the coverage and capacity of integrated multiple-HAP 3G systems, and improving the energy efficiency of cooperative wireless sensor networks. The performance of these systems is assessed by theoretical analysis, by computer simulations under a range of propagation environments including realistic channel models, advanced commercial electromagnetic modeling software, and a proposed novel multichannel simulator suitable for various space-time applications. space-time processing applications for wireless communications ABSTRACT Tommy Hult View publication stats ISSN 1653-2090 ISBN 978-91-7295-146-4 2008:12 2008:12 space-time processing applications for wireless communications Tommy Hult Blekinge Institute of Technology Doctoral Dissertation Series No. 2008:12 School of Engineering