Particle Detector (PD) Experiment of the Korea Space Environment Monitor (KSEM) Aboard Geostationary Satellite GK2A

被引:0
作者
J. Seon
K.-S. Chae
G. W. Na
H.-K. Seo
Y.-C. Shin
J. Woo
C.-H. Lee
W.-H. Seol
C.-A. Lee
S. Pak
H. Lee
S.-H. Shin
D. E. Larson
K. Hatch
G. K. Parks
J. Sample
M. McCarthy
C. Tindall
Y.-J. Jeon
J.-K. Choi
J.-Y. Park
机构
[1] Kyung Hee University,School of Space Research
[2] University of California,Space Science Laboratory
[3] Montana State University,Department of Physics
[4] University of Washington,Department of Earth and Space Science
[5] Lawrence Berkeley Laboratory,undefined
[6] Satrec Initiative Co.,undefined
来源
Space Science Reviews | 2020年 / 216卷
关键词
Space weather; Geostationary orbit; Radiation belt; Charged particle detector; Silicon detectors;
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摘要
The Particle Detector (PD) experiment aboard the geostationary satellite GEO-KOMPSAT-2A (GK2A) measures populations of electrons and positive ions in the Earth’s geostationary orbit at a geographic longitude of 128.2∘E\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$128.2^{\circ }\mbox{E}$\end{document}, inclination of 0∘\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$0^{\circ }$\end{document} and a mean orbital radius of 6.6 Earth radii (RE\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$R_{E}$\end{document}). The PD experiment consists of three sensors with different viewing angles relative to the spacecraft. Each sensor consists of two telescopes that are mechanically configured back-to-back with a field-of-view of 20∘×20∘\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$20^{\circ }\times 20^{\circ }$\end{document} and measures electrons and ions, using silicon detectors equipped with foils and magnets for the separation of ions and electrons. The energy ranges of the sensor for electrons and ions are 100–3800 keV and 148–22500 keV, respectively. A particular emphasis on electron measurement is given by allocating 48 energy bins in the measured energy range, whereas 22 energy bins are allocated for ion measurements. This unprecedented energy resolution of ΔE/E\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$\Delta E/E$\end{document} in the range 5–25% for the electron and ion flux measurements is acquired every three seconds with cyclic polling of each sensor every second to provide an effective temporal resolution of one second. Together with the magnetometer aboard the spacecraft, the PD experiment will provide quantitative observations that will enable improved understanding of the adiabatic and nonadiabatic dynamics of the Earth’s magnetosphere for space weather studies at geostationary orbits from the vantage point of a far-east longitude.
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  • [1] Agostinelli S.(2003)Geant4—a simulation toolkit Nucl. Instrum. Methods Phys. Res., Sect. A, Accel. Spectrom. Detect. Assoc. Equip. 506 250-303
  • [2] Allison J.(2006)Geant4 developments and applications IEEE Trans. Nucl. Sci. 53 270-278
  • [3] Amako K.(1969)Particle substorms observed at the geostationary orbit J. Geophys. Res. 74 5019-5028
  • [4] Apostolakis J.(1982)Observation and modeling of energetic particles at synchronous orbit on July 29, 1977 J. Geophys. Res. Space Phys. 87 5917-5932
  • [5] Araujo H.(1978)High-resolution energetic particle measurements at 6.6 RE, 2. High-energy proton drift echoes J. Geophys. Res. Space Phys. 83 4857-4862
  • [6] Arce P.(1969)Response of silicon detectors to monoenergetic electrons with energies between 0.15 and 5.0 MeV Nucl. Instrum. Methods 69 181-193
  • [7] Asai M.(1973)Nightside energetic particle decreases at the synchronous orbit J. Geophys. Res. 78 8119-8127
  • [8] Axen D.(1968)Magnetic fields in the magnetopause and vicinity at synchronous altitude J. Geophys. Res. 73 5699-5718
  • [9] Banerjee S.(2015)The maven solar energetic particle investigation Space Sci. Rev. 195 153-172
  • [10] Barrand G.(1978)Low-energy plasma observations at synchronous orbit J. Geophys. Res. Space Phys. 83 2145-2156