TY - JOUR
T1 - Planet-C
T2 - Venus Climate Orbiter mission of Japan
AU - Nakamura, Masato
AU - Imamura, Takeshi
AU - Ueno, Munetaka
AU - Iwagami, Naomoto
AU - Satoh, Takehiko
AU - Watanabe, Shigeto
AU - Taguchi, Makoto
AU - Takahashi, Yukihiro
AU - Suzuki, Makoto
AU - Abe, Takumi
AU - Hashimoto, George L.
AU - Sakanoi, Takeshi
AU - Okano, Shoichi
AU - Kasaba, Yasumasa
AU - Yoshida, Jun
AU - Yamada, Manabu
AU - Ishii, Nobuaki
AU - Yamada, Takahiro
AU - Uemizu, Kazunori
AU - Fukuhara, Tetsuya
AU - Oyama, Koh ichiro
PY - 2007/10
Y1 - 2007/10
N2 - The Venus Climate Orbiter mission (PLANET-C), one of the future planetary missions of Japan, aims at understanding the atmospheric circulation of Venus. Meteorological information will be obtained by globally mapping clouds and minor constituents successively with four cameras at ultraviolet and infrared wavelengths, detecting lightning with a high-speed imager, and observing the vertical structure of the atmosphere with radio science technique. The equatorial elongated orbit with westward revolution fits the observation of the movement and temporal variation of the atmosphere which as a whole rotates westward. The systematic, continuous imaging observations will provide us with an unprecedented large data set of the Venusian atmospheric dynamics. Additional targets of the mission are the exploration of the ground surface and the observation of zodiacal light. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.
AB - The Venus Climate Orbiter mission (PLANET-C), one of the future planetary missions of Japan, aims at understanding the atmospheric circulation of Venus. Meteorological information will be obtained by globally mapping clouds and minor constituents successively with four cameras at ultraviolet and infrared wavelengths, detecting lightning with a high-speed imager, and observing the vertical structure of the atmosphere with radio science technique. The equatorial elongated orbit with westward revolution fits the observation of the movement and temporal variation of the atmosphere which as a whole rotates westward. The systematic, continuous imaging observations will provide us with an unprecedented large data set of the Venusian atmospheric dynamics. Additional targets of the mission are the exploration of the ground surface and the observation of zodiacal light. The mission will complement the ESA's Venus Express, which also explores the Venusian environment with different approaches.
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U2 - 10.1016/j.pss.2007.01.009
DO - 10.1016/j.pss.2007.01.009
M3 - Article
AN - SCOPUS:34548204458
SN - 0032-0633
VL - 55
SP - 1831
EP - 1842
JO - Planetary and Space Science
JF - Planetary and Space Science
IS - 12
ER -