2021 IEEE 3rd Eurasia Conference on IOT, Communication and Engineering (ECICE), Oct 29, 2021
With the development of network technology, the industry has improved product quality and product... more With the development of network technology, the industry has improved product quality and productivity by adopting digitalization and automated testing and production through the Internet of Things (IoT). As every household uses electricity, it has an electricity meter to measure the amount of electric energy. Taiwan Power Company has installed electricity meters with a mechanical and analog system. However, smart technology needs to be introduced to the meter, which replaces the existing ones. However, it is a waste of resources to discard tens of millions of previous meters, which does not meet the needs of a circular economy. Therefore, it is required to find a way to use the previous electric meters with an innovative and creative adjustment. This research verifies the possibility of recycling the glass cover of the mechanical analog meter to cooking glassware. The composition of the glass cover and heavy metal analysis of dirt on the surface revealed that it is appropriate for cooking and heating. The test results show that the glass cover is suitable for cooking in a microwave oven but not on an electric ceramic cooker (hot plate). In conclusion, this study proposes a possibility to recycle the glass cover after cleaning and attaching a new logo.
The Pan-STARRS project is operated by an international consortium. Located in Haleakala, Hawaii, ... more The Pan-STARRS project is operated by an international consortium. Located in Haleakala, Hawaii, the Pan-STARRS telescope system patrols the entire visible sky several times a month, with an aim to identify and characterize varying celestial objects of phenomena or in brightness (supernovae, novae, variable stars, etc) or in position (comets, asteroids, near-earth objects, X-planet etc.) PS1 science mission has started officially from May, 2010 and expects to end in the end of 2013. As of early 2012, every patch of sky observable from Hawaii has been observed in at least 5 bands (g’, r’, i’, z’, y’) for 5 to 40 epochs. We have set up a data depository at NCU to serve the users in Taiwan. The massive amounts of Pan-STARRS data are downloaded via Internet from the Institute for Astronomy, University of Hawaii whenever new observations are obtained and processed. So far we have stored a total of 200 TB worth of data. In addition to star/galaxy catalogs, a postage stamp server provides access to FITS images. ...
We present the star formation activity around the emission nebula Sh2-112. At a distance of ∼2.1 ... more We present the star formation activity around the emission nebula Sh2-112. At a distance of ∼2.1 kpc, this H ii complex, itself 3 pc in radius, is illuminated by the massive star (O8 V) BD+45 3216. The associated molecular cloud extends in angular scales of 2.°0 × 0.°83, corresponding to linear sizes of 73 pc by 30 pc, along the Galactic longitude. The high-resolution (30″) extinction map reveals a chain of dust clumps aligned with the filament-like structure with an average extinction of A V ∼ 2.78 mag, varying up to a maximum of ∼17 mag. Our analysis led to identification of a rich population (∼500) of young (average age of ∼1 Myr) stars, plus a numerous number (∼350) of Hα emitters, spatially correlated with the filamentary clouds. Located near the edge of the cloud, the luminous star BD+45 3216 has created an arc-like pattern as the ionizing radiation encounters the dense gas, forming a blister-shaped morphology. We found three distinct young stellar groups, all coincident with relatively dense parts of the cloud complex, signifying ongoing star formation. Moreover, the cloud filament (excitation temperature ∼10 K) traced by the CO isotopologues and extending nearly ∼80 pc is devoid of ionized gas except at the dense cores (excitation temperature ∼28–32 K) wherein significant ionized emission excited by OB stars (dynamical age ∼0.18–1.0 Myr) pertains. The radial velocity is dynamic (median ∼−3.65 km s−1) along the main filament, increasing from Galactic east to west, indicating mass flow to form the massive stars/clusters at the central hubs.
Astrophysical Journal Supplement Series, Dec 13, 2022
We present Gemini-NIFS, Very Large Telescope-SINFONI, and Keck-OSIRIS observations of near-IR [Fe... more We present Gemini-NIFS, Very Large Telescope-SINFONI, and Keck-OSIRIS observations of near-IR [Fe ii] emission that are associated with well-studied jets from three active T Tauri stars—RW Aur A, RY Tau, and DG Tau—taken from 2012 to 2021. We primarily cover the redshifted jet from RW Aur A and the blueshifted jets from RY Tau and DG Tau, in order to investigate long-term time variabilities that are potentially related to the activities of mass accretion and/or the stellar magnetic fields. All of these jets consist of several moving knots, with tangential velocities of 70–240 km s−1, which were ejected from the star with different velocities and at irregular time intervals. Via comparisons with the literature, we identify significant differences in the tangential velocities between 1985–2008 and 2008–2021 for the DG Tau jet. The sizes of the individual knots appear to increase with time, and, in turn, their peak brightnesses in the 1.644 μm emission decreased by up to a factor of ∼30 during the epochs of our observations. The variety of decay timescales measured in the [Fe ii] 1.644 μm emission could be attributed to different preshock conditions should the moving knots be unresolved shocks. However, our data do not exclude the possibility that these knots are due to nonuniform density/temperature distributions with another heating mechanism, or, in some cases, due to stationary shocks without proper motions. Spatially resolved observations of these knots with significantly higher angular resolutions will be necessary to better understand their physical nature.
2021 IEEE 3rd Eurasia Conference on IOT, Communication and Engineering (ECICE), Oct 29, 2021
With the development of network technology, the industry has improved product quality and product... more With the development of network technology, the industry has improved product quality and productivity by adopting digitalization and automated testing and production through the Internet of Things (IoT). As every household uses electricity, it has an electricity meter to measure the amount of electric energy. Taiwan Power Company has installed electricity meters with a mechanical and analog system. However, smart technology needs to be introduced to the meter, which replaces the existing ones. However, it is a waste of resources to discard tens of millions of previous meters, which does not meet the needs of a circular economy. Therefore, it is required to find a way to use the previous electric meters with an innovative and creative adjustment. This research verifies the possibility of recycling the glass cover of the mechanical analog meter to cooking glassware. The composition of the glass cover and heavy metal analysis of dirt on the surface revealed that it is appropriate for cooking and heating. The test results show that the glass cover is suitable for cooking in a microwave oven but not on an electric ceramic cooker (hot plate). In conclusion, this study proposes a possibility to recycle the glass cover after cleaning and attaching a new logo.
The Pan-STARRS project is operated by an international consortium. Located in Haleakala, Hawaii, ... more The Pan-STARRS project is operated by an international consortium. Located in Haleakala, Hawaii, the Pan-STARRS telescope system patrols the entire visible sky several times a month, with an aim to identify and characterize varying celestial objects of phenomena or in brightness (supernovae, novae, variable stars, etc) or in position (comets, asteroids, near-earth objects, X-planet etc.) PS1 science mission has started officially from May, 2010 and expects to end in the end of 2013. As of early 2012, every patch of sky observable from Hawaii has been observed in at least 5 bands (g’, r’, i’, z’, y’) for 5 to 40 epochs. We have set up a data depository at NCU to serve the users in Taiwan. The massive amounts of Pan-STARRS data are downloaded via Internet from the Institute for Astronomy, University of Hawaii whenever new observations are obtained and processed. So far we have stored a total of 200 TB worth of data. In addition to star/galaxy catalogs, a postage stamp server provides access to FITS images. ...
We present the star formation activity around the emission nebula Sh2-112. At a distance of ∼2.1 ... more We present the star formation activity around the emission nebula Sh2-112. At a distance of ∼2.1 kpc, this H ii complex, itself 3 pc in radius, is illuminated by the massive star (O8 V) BD+45 3216. The associated molecular cloud extends in angular scales of 2.°0 × 0.°83, corresponding to linear sizes of 73 pc by 30 pc, along the Galactic longitude. The high-resolution (30″) extinction map reveals a chain of dust clumps aligned with the filament-like structure with an average extinction of A V ∼ 2.78 mag, varying up to a maximum of ∼17 mag. Our analysis led to identification of a rich population (∼500) of young (average age of ∼1 Myr) stars, plus a numerous number (∼350) of Hα emitters, spatially correlated with the filamentary clouds. Located near the edge of the cloud, the luminous star BD+45 3216 has created an arc-like pattern as the ionizing radiation encounters the dense gas, forming a blister-shaped morphology. We found three distinct young stellar groups, all coincident with relatively dense parts of the cloud complex, signifying ongoing star formation. Moreover, the cloud filament (excitation temperature ∼10 K) traced by the CO isotopologues and extending nearly ∼80 pc is devoid of ionized gas except at the dense cores (excitation temperature ∼28–32 K) wherein significant ionized emission excited by OB stars (dynamical age ∼0.18–1.0 Myr) pertains. The radial velocity is dynamic (median ∼−3.65 km s−1) along the main filament, increasing from Galactic east to west, indicating mass flow to form the massive stars/clusters at the central hubs.
Astrophysical Journal Supplement Series, Dec 13, 2022
We present Gemini-NIFS, Very Large Telescope-SINFONI, and Keck-OSIRIS observations of near-IR [Fe... more We present Gemini-NIFS, Very Large Telescope-SINFONI, and Keck-OSIRIS observations of near-IR [Fe ii] emission that are associated with well-studied jets from three active T Tauri stars—RW Aur A, RY Tau, and DG Tau—taken from 2012 to 2021. We primarily cover the redshifted jet from RW Aur A and the blueshifted jets from RY Tau and DG Tau, in order to investigate long-term time variabilities that are potentially related to the activities of mass accretion and/or the stellar magnetic fields. All of these jets consist of several moving knots, with tangential velocities of 70–240 km s−1, which were ejected from the star with different velocities and at irregular time intervals. Via comparisons with the literature, we identify significant differences in the tangential velocities between 1985–2008 and 2008–2021 for the DG Tau jet. The sizes of the individual knots appear to increase with time, and, in turn, their peak brightnesses in the 1.644 μm emission decreased by up to a factor of ∼30 during the epochs of our observations. The variety of decay timescales measured in the [Fe ii] 1.644 μm emission could be attributed to different preshock conditions should the moving knots be unresolved shocks. However, our data do not exclude the possibility that these knots are due to nonuniform density/temperature distributions with another heating mechanism, or, in some cases, due to stationary shocks without proper motions. Spatially resolved observations of these knots with significantly higher angular resolutions will be necessary to better understand their physical nature.
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Papers by Wen-Ping Chen