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Volumn 154, Issue 1-4, 2010, Pages 305-316

Studying the lunar ionosphere with SELENE radio science experiment

(14) Imamura, Takeshi a Iwata, Takahiro a Yamamoto, Zen Ichi a Mochizuki, Nanako a Kono, Yusuke b Matsumoto, Koji b Liu, Qinghui c Noda, Hirotomo b Hanada, Hideo b Oyama, Koh Ichiro d Nabatov, Alexander e Futaana, Yoshifumi f Saito, Akinori g Ando, Hiroki h

a JAPAN AEROSPACE EXPLORATION AGENCY (Japan)

b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN (Japan)

c CHINESE ACADEMY OF SCIENCES (China)

d NATIONAL CENTRAL UNIVERSITY (Taiwan)

e INSTITUTE OF HYDROBIOLOGY (Ukraine)

f SWEDISH INSTITUTE OF SPACE PHYSICS (Sweden)

g KYOTO UNIVERSITY (Japan)

h UNIVERSITY OF TOKYO (Japan)

Author keywords

Ionosphere; Kaguya; Moon; Radio occultation; SELENE

Indexed keywords

ELECTRON DENSITIES; ERROR SOURCES; GENERATION MECHANISM; KAGUYA; LUNAR SURFACE; PEAK DENSITY; RADIO OCCULTATION; RADIO OCCULTATION MEASUREMENTS; RADIO OCCULTATIONS; RADIO SCIENCE; RAY PATHS; SELENE; STATISTICAL ANALYSIS; WEAK SIGNALS;

IONOSPHERE; IONOSPHERIC MEASUREMENT; RADIO; SOLAR WIND;

LUNAR MISSIONS;

EID: 78650170916 PISSN: 00386308 EISSN: 15729672 Source Type: Journal
DOI: 10.1007/s11214-010-9660-0 Document Type: Article

Times cited : (15)

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