講演抄録/キーワード |
講演名 |
2010-10-28 09:20
[招待講演]Remote sensors mounted on AKATSUKI ○Masato Nakamura・Nobuaki Ishii・Takeshi Imamura・Makoto Suzuki・Munetaka Ueno・Atsushi Yamazaki・Takehiko Satoh(ISAS)・Naomoto Iwagami(Univ. of Tokyo)・Makoto Taguchi(Rikkyo Univ.)・Shigeto Watanabe・Yukihiro Takahashi・Tetsuya Fukuhara(Hokkaido Univ.)・Shoko Ohtsuki(ISAS) SANE2010-91 |
抄録 |
(和) |
Japanese Venus Climate Orbiter 'AKATSUKI' (PLANET-C) was successfully launched at 06:58:22JST on May 21, by H-IIA F17. After the separation from H-IIA, the telemetry from AKATSUKI was normally detected by DSN Goldstone station (10:00JST) and the solar cell paddles' expansion was confirmed. AKATSUKI was put into the 3-axis stabilized mode in the initial operation from Uchinoura station and the critical operation was finished at 20:00JST on the same day.
AKATSUKI will arrive at Venus on Dec 7, 2010. From the orbit around Venus, it will take pictures of the distribution of clouds and minor gas components at different wavelength by 4 cameras. These data will be analyzed to study the meteorology on Venus, especially the mechanism of the super-rotaion of Venusian atmosphere which is still the top mystery of the Venus science. Simultaneous observation with ESA's Venus Express is highly expected to study the Venusian atmosphere.
We will present the development of those remote sensing equipments in our talk. |
(英) |
Japanese Venus Climate Orbiter 'AKATSUKI' (PLANET-C) was successfully launched at 06:58:22JST on May 21, by H-IIA F17. After the separation from H-IIA, the telemetry from AKATSUKI was normally detected by DSN Goldstone station (10:00JST) and the solar cell paddles' expansion was confirmed. AKATSUKI was put into the 3-axis stabilized mode in the initial operation from Uchinoura station and the critical operation was finished at 20:00JST on the same day.
AKATSUKI will arrive at Venus on Dec 7, 2010. From the orbit around Venus, it will take pictures of the distribution of clouds and minor gas components at different wavelength by 4 cameras. These data will be analyzed to study the meteorology on Venus, especially the mechanism of the super-rotaion of Venusian atmosphere which is still the top mystery of the Venus science. Simultaneous observation with ESA's Venus Express is highly expected to study the Venusian atmosphere.
We will present the development of those remote sensing equipments in our talk. |
キーワード |
(和) |
Venus / Exploration / / / / / / |
(英) |
Venus / Exploration / / / / / / |
文献情報 |
信学技報, vol. 110, no. 250, SANE2010-91, pp. 137-140, 2010年10月. |
資料番号 |
SANE2010-91 |
発行日 |
2010-10-20 (SANE) |
ISSN |
Print edition: ISSN 0913-5685 Online edition: ISSN 2432-6380 |
著作権に ついて |
技術研究報告に掲載された論文の著作権は電子情報通信学会に帰属します.(許諾番号:10GA0019/12GB0052/13GB0056/17GB0034/18GB0034) |
PDFダウンロード |
SANE2010-91 |