Abstract
The Sun is an effective particle accelerator that produces solar energetic particle (SEP) events, during which particles of up to several GeVs can be observed. These events, when they are observed at Earth with the neutron monitor network, are called ground-level enhancements (GLEs). Although these events with their high-energy component have been investigated for several decades, a clear relation between the spectral shape of the SEPs outside the Earth’s magnetosphere and the increase in neutron monitor count rate has yet to be established. Hence, an analysis of these events is of interest for the space weather and for the solar event community.
In this article, SEP events with protons accelerated to above 500 MeV were identified using data obtained with the Electron Proton Helium Instrument (EPHIN) onboard the Solar and Heliospheric Observatory (SOHO) between 1995 and 2015. For a statistical analysis, onset times were determined for the events and the proton energy spectra were derived and fitted with a power law.
As a result, we present a list of 42 SEP events with protons accelerated to above 500 MeV measured with the EPHIN instrument onboard SOHO. The statistical analysis based on the fitted spectral slopes and absolute intensities is discussed, with special emphasis on whether an event has been observed as a GLE. Furthermore, we are able to determine that the derived intensity at 500 MeV and the observed increase in neutron monitor count rate are correlated for a subset of events.
Similar content being viewed by others
References
Band, D., Matteson, J., Ford, L., Schaefer, B., Palmer, D., Teegarden, B., Cline, T., Briggs, M., Paciesas, W., Pendleton, G., Fishman, G., Kouveliotou, C., Meegan, C., Wilson, R., Lestrade, P.: 1993, BATSE observations of gamma-ray burst spectra. I – Spectral diversity. Astrophys. J. 413, 281. DOI .
Cane, H.V.: 2000, Coronal mass ejections and Forbush decreases. Space Sci. Rev. 93, 55. DOI .
Cliver, E.W.: 2006, The unusual relativistic solar proton events of 1979 August 21 and 1981 May 10. Astrophys. J. 639, 1206. DOI .
Cliver, E.W., Kahler, S.W., Cane, H.V., Koomen, M.J., Michels, D.J., Howard, R.A., Sheeley, N.R. Jr.: 1983, The GLE-associated flare of 21 August, 1979. Solar Phys. 89, 181. DOI . ADS .
Danilova, O.: 1999, The GLE of May 2, 1998: An effect of disturbed magnetosphere on solar cosmic rays. In: Int. Cosmic Ray Conf. 6, 399. ADS .
Forbush, S.E.: 1946, Three unusual cosmic-ray increases possibly due to charged particles from the Sun. Phys. Rev. 70, 771. DOI .
GEANT4 collaboration: 2006, An object-oriented toolkit for simulation in hep. CERN-LHCC 98-44. See also http://geant4.cern.ch/ .
Gopalswamy, N., Mäkelä, P.: 2014, Latitudinal connectivity of ground level enhancement events. In: Hu, Q., Zank, G.P. (eds.) Outstanding Problems in Heliophysics: From Coronal Heating to the Edge of the Heliosphere, Astron. Soc. Pacific Conf. Ser. 484, 63. ADS .
Gopalswamy, N., Mäkelä, P., Yashiro, S., Xie, H., Akiyama, S., Thakur, N.: 2015, High-energy solar particle events in cycle 24. J. Phys. Conf. Ser. 642(1), 012012. DOI .
Hanser, F.A.: 2011, EPS/HEPAD calibration and data handbook. Tech. rep. goesn-eng-048d. Available at www.ngdc.noaa.gov/stp/satellite/goes/documentation.html . DOI .
Heber, B., Fichtner, H., Scherer, K.: 2006, Solar and heliospheric modulation of galactic cosmic rays. Space Sci. Rev. 125, 81. DOI . ADS .
Heber, B., Potgieter, M.S.: 2006, Cosmic rays at high heliolatitudes. Space Sci. Rev. 127, 117. DOI . ADS .
Heber, B., Dresing, N., Herbst, K., Klassen, A., Kühl, P., Gómez-Herrero, R.: 2015, Proton energy spectra during ground level enhancements as measured by EPHIN aboard SOHO. In: Proc. Science ICRC 2015.
Kühl, P., Gómez-Herrero, R., Heber, B.: 2016, Annual cosmic ray spectra from 250 MeV up to 1.6 GeV from 1995 – 2014 measured with the electron proton helium instrument onboard SOHO. Solar Phys. 291, 965. DOI .
Kühl, P., Banjac, S., Dresing, N., Gómez-Herrero, R., Heber, B., Klassen, A., et al.: 2015a, Proton intensity spectra during the solar energetic particle events of May 17, 2012 and January 6, 2014. Astron. Astrophys. 576, A120. DOI . ADS .
Kühl, P., Dresing, N., Gieseler, J., Heber, B., Klassen, A.: 2015b, Galactic cosmic ray spectra during solar cycle 23 and 24 – Measurement capabilities of the electron proton helium instrument. In: Proc. Science ICRC 2015.
Lockwood, J.A., Debrunner, H.: 1999, Solar flare particle measurements with neutron monitors. Space Sci. Rev. 88, 483. DOI . ADS .
McCracken, K.G., Freon, A.: 1962, Asymptotic directions and cut-off rigidities in the geomagnetic field. J. Phys. Soc. Japan 17, AII, 455. ADS .
McCracken, K.G., Moraal, H., Shea, M.A.: 2012, The high-energy impulsive ground-level enhancement. Astrophys. J. 761, 101. DOI .
McGuire, R.E., von Rosenvinge, T.T. McDonald, F.B.: 1986, The composition of solar energetic particles. Astrophys. J. 301, 938. DOI .
Mewaldt, R.A., Looper, M.D., Cohen, C.M.S., Haggerty, D.K., Labrador, A.W., Leske, R.A., Mason, G.M., Mazur, J.E., von Rosenvinge, T.T.: 2012, Energy spectra, composition, and other properties of ground-level events during solar cycle 23. Space Sci. Rev. 171, 97. DOI .
Mishev, A.L., Usoskin, I.G., Kovaltsov, G.A.: 2013, Neutron monitor yield function: New improved computations. J. Geophys. Res. 118, 2783. DOI . ADS .
Müller-Mellin, R., Kunow, H., Fleißner, V., Pehlke, E., Rode, E., Röschmann, N., et al.: 1995, Costep – Comprehensive suprathermal and energetic particle analyser. Solar Phys. 162, 483.
Nitta, N.V., Liu, Y., DeRosa, M.L., Nightingale, R.W.: 2012, What are special about ground-level events? Flares, CMEs, active regions and magnetic field connection. Space Sci. Rev. 171, 61. DOI . ADS .
Nymmik, R.: 1999, Relationships among solar activity SEP occurrence frequency, and solar energetic particle event distribution function. In: Int. Cosmic Ray Conf., 6, 280. ADS .
Onsager, T., Grubb, R., Kunches, J., Matheson, L., Speich, D., Zwickl, R.W., Sauer, H.: 1996, Operational uses of the GOES energetic particle detectors. In: Washwell, E.R. (ed.) GOES-8 and Beyond, Proc. SPIE 2812, 281. DOI .
Plainaki, C., Mavromichalaki, H., Belov, A., Eroshenko, E., Yanke, V.: 2009, Modeling the solar cosmic ray event of 13 December 2006 using ground level neutron monitor data. Adv. Space Res. 43, 474. DOI . ADS .
Reames, D.V.: 2013, The two sources of solar energetic particles. Space Sci. Rev. 175, 53. DOI . ADS .
Sandberg, I., Jiggens, P., Heynderickx, D., Daglis, I.A.: 2014, Cross calibration of NOAA GOES solar proton detectors using corrected NASA IMP-8/GME data. Geophys. Res. Lett. 41, 4435. DOI . ADS .
Shen, C., Li, G., Kong, X., Hu, J., Sun, X.D., Ding, L., Chen, Y., Wang, Y., Xia, L.: 2013, Compound twin coronal mass ejections in the 2012 May 17 GLE event. Astrophys. J. 763, 114. DOI . ADS .
Smart, D.F., Shea, M.A., Flückiger, E.O.: 2000, Magnetospheric models and trajectory computations. Space Sci. Rev. 93, 305. DOI . ADS .
Thakur, N., Gopalswamy, N., Xie, H., Mäkelä, P., Yashiro, S., Akiyama, S., Davila, J.M.: 2014, Ground level enhancement in the 2014 January 6 solar energetic particle event. Astrophys. J. Lett. 790, L13. DOI . ADS .
Thakur, N., Gopalswamy, N., Mäkelä, P., Akiyama, S., Yashiro, S., Xie, H.: 2016, Two exceptions in the large SEP events of solar cycles 23 and 24. Solar Phys. 291, 513. DOI .
Tylka, A.J., Cohen, C.M.S., Dietrich, W.F., Lee, M.A., Maclennan, C.G., Mewaldt, R.A., Ng, C.K., Reames, D.V.: 2006, A comparative study of ion characteristics in the large gradual solar energetic particle events of 2002 April 21 and 2002 August 24. Astrophys. J. Suppl. 164, 536. DOI . ADS .
Vainio, R., Valtonen, E., Heber, B., Malandraki, O.E., Papaioannou, A., Klein, K.-L., Afanasiev, A., Agueda, N., Aurass, H., Battarbee, M., Braune, S., Dröge, W., Ganse, U., Hamadache, C., Heynderickx, D., Huttunen-Heikinmaa, K., Kiener, J., Kilian, P., Kopp, A., Kouloumvakos, A., Maisala, S., Mishev, A., Miteva, R., Nindos, A., Oittinen, T., Raukunen, O., Riihonen, E., Rodríguez-Gasén, R., Saloniemi, O., Sanahuja, B., Scherer, R., Spanier, F., Tatischeff, V., Tziotziou, K., Usoskin, I.G., Vilmer, N.: 2013, The first SEPServer event catalogue \({\sim\,}68\mbox{-MeV}\) solar proton events observed at 1 AU in 1996 – 2010. J. Space Weather Space Clim. 3(27), A12. DOI .
Acknowledgements
The SOHO/EPHIN project is supported under Grant 50 OC 1302 by the German Bundesministerium für Wirtschaft through the Deutsches Zentrum für Luft- und Raumfahrt (DLR).
This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No. 637324.
This work was carried out within the framework of the bilateral BMBF-NRF-project ‘Astrohel’ (01DG15009) funded by the Bundesministerium für Bildung und Forschung. The responsibility of the contents of this work is with the authors.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Disclosure of Potential Conflicts of Interest
The authors declare that they have no conflicts of interest.
Rights and permissions
About this article
Cite this article
Kühl, P., Dresing, N., Heber, B. et al. Solar Energetic Particle Events with Protons Above 500 MeV Between 1995 and 2015 Measured with SOHO/EPHIN. Sol Phys 292, 10 (2017). https://doi.org/10.1007/s11207-016-1033-8
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s11207-016-1033-8