Low-energy charged particle measurement by MAP-PACE onboard SELENE

被引:0
|
作者
Yoshifumi Saito
Shoichiro Yokota
Kazushi Asamura
Takaaki Tanaka
Ryota Akiba
Masaki Fujimoto
Hiroshi Hasegawa
Hajime Hayakawa
Masafumi Hirahara
Masahiro Hoshino
Shinobu Machida
Toshifumi Mukai
Tsugunobu Nagai
Tsutomu Nagatsuma
Masato Nakamura
Koh-ichiro Oyama
Eiichi Sagawa
Susumu Sasaki
Kanako Seki
Toshio Terasawa
机构
[1] Japan Aerospace Exploration Agency,Institute of Space and Astronautical Science
[2] Hamagin Research Institute,Solar
[3] Ltd.,Terrestrial Environment Laboratory
[4] University of Tokyo,undefined
[5] Kyoto University,undefined
[6] Tokyo Institute of Technology,undefined
[7] National Institute of Information and Communications Technology,undefined
[8] Research Institute of Telecommunications and Economics,undefined
[9] Nagoya University,undefined
来源
Earth, Planets and Space | 2008年 / 60卷
关键词
Moon; plasma; magnetic anomaly; alkali atmosphere; magnetosphere; solar wind;
D O I
暂无
中图分类号
学科分类号
摘要
MAP-PACE (MAgnetic field and Plasma experiment-Plasma energy Angle and Composition Experiment) is one of the scientific instruments onboard the SELENE (SELenological and ENgineering Explorer) satellite. PACE consists of four sensors: ESA (Electron Spectrum Analyzer)-S1, ESA-S2, IMA (Ion Mass Analyzer), and IEA (Ion Energy Analyzer). ESA-S1 and S2 measure the distribution function of low-energy electrons below 15 keV, while IMA and IEA measure the distribution function of low energy ions below 28 keV/q. Each sensor has a hemispherical field of view. Since SELENE is a three-axis stabilized spacecraft, a pair of electron sensors (ESA-S1 and S2) and a pair of ion sensors (IMA and IEA) are necessary for obtaining a three-dimensional distribution function of electrons and ions. The scientific objectives of PACE are (1) to measure the ions sputtered from the lunar surface and the lunar atmosphere, (2) to measure the magnetic anomaly on the lunar surface using two ESAs and a magnetometer onboard SELENE simultaneously as an electron reflectometer, (3) to resolve the Moon-solar wind interaction, (4) to resolve the Moon-Earth’s magnetosphere interaction, and (5) to observe the Earth’s magnetotail.
引用
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页码:375 / 385
页数:10
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