Low-energy charged particle measurement by MAP-PACE onboard SELENE
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Published:2008-04
Issue:4
Volume:60
Page:375-385
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ISSN:1880-5981
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Container-title:Earth, Planets and Space
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language:en
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Short-container-title:Earth Planet Sp
Author:
Saito Yoshifumi,Yokota Shoichiro,Asamura Kazushi,Tanaka Takaaki,Akiba Ryota,Fujimoto Masaki,Hasegawa Hiroshi,Hayakawa Hajime,Hirahara Masafumi,Hoshino Masahiro,Machida Shinobu,Mukai Toshifumi,Nagai Tsugunobu,Nagatsuma Tsutomu,Nakamura Masato,Oyama Koh-ichiro,Sagawa Eiichi,Sasaki Susumu,Seki Kanako,Terasawa Toshio
Abstract
Abstract
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.
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Geology
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