TY - JOUR
T1 - First in situ observation of the Moon-originating ions in the Earth's Magnetosphere by MAP-PACE on SELENE (KAGUYA)
AU - Tanaka, Takaaki
AU - Saito, Yoshifumi
AU - Yokota, Shoichiro
AU - Asamura, Kazushi
AU - Nishino, Masaki N.
AU - Tsunakawa, Hideo
AU - Shibuya, Hidetoshi
AU - Matsushima, Masaki
AU - Shimizu, Hisayoshi
AU - Takahashi, Futoshi
AU - Fujimoto, Masaki
AU - Mukai, Toshifumi
AU - Terasawa, Toshio
N1 - Copyright:
Copyright 2010 Elsevier B.V., All rights reserved.
PY - 2009/11
Y1 - 2009/11
N2 - In contrast to many ground-based optical observations of the thin lunar alkali exosphere, in situ observations of the exospheric ions by satellite-borne plasma instruments have been quite rare. MAP-PACE-IMA onboard Japanese lunar orbiter SELENE (KAGUYA) succeeded in detecting Moon originating ions at 100 km altitude. Here we make the first report of the ion detection during intervals when the Moon was embedded in the Earth's magnetotail lobe. In the absence of plasma effects on the source process, ion species of H+, He ++, He+, C+, O+, Na+, K+ and Ar+ are definitively identified. The ion fluxes were higher when the solar zenith angle was smaller, which is consistent with the idea that the solar photon driven processes dominates in supplying exospheric components.
AB - In contrast to many ground-based optical observations of the thin lunar alkali exosphere, in situ observations of the exospheric ions by satellite-borne plasma instruments have been quite rare. MAP-PACE-IMA onboard Japanese lunar orbiter SELENE (KAGUYA) succeeded in detecting Moon originating ions at 100 km altitude. Here we make the first report of the ion detection during intervals when the Moon was embedded in the Earth's magnetotail lobe. In the absence of plasma effects on the source process, ion species of H+, He ++, He+, C+, O+, Na+, K+ and Ar+ are definitively identified. The ion fluxes were higher when the solar zenith angle was smaller, which is consistent with the idea that the solar photon driven processes dominates in supplying exospheric components.
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U2 - 10.1029/2009GL040682
DO - 10.1029/2009GL040682
M3 - Article
AN - SCOPUS:72049120650
SN - 0094-8276
VL - 36
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 22
M1 - L22106
ER -