Performance of Akatsuki/IR2 in Venus orbit: the first year-Reference-Cited by-同舟云学术

Performance of Akatsuki/IR2 in Venus orbit: the first year

Published:2017-11-03 Issue:1 Volume:69 Page:
ISSN:1880-5981
Container-title:Earth, Planets and Space
language:en
Short-container-title:Earth Planets Space

Author:

Satoh Takehiko^ORCID,Sato Takao M.,Nakamura Masato,Kasaba Yasumasa,Ueno Munetaka,Suzuki Makoto,Hashimoto George L.,Horinouchi Takeshi,Imamura Takeshi,Yamazaki Atsushi,Enomoto Takayuki,Sakurai Yuri,Takami Kosuke,Sawai Kenta,Nakakushi Takashi,Abe Takumi,Ishii Nobuaki,Hirose Chikako,Hirata Naru,Yamada Manabu,Murakami Shin-ya,Yamamoto Yukio,Fukuhara Tetsuya,Ogohara Kazunori,Ando Hiroki,Sugiyama Ko-ichiro,Kashimura Hiroki,Ohtsuki Shoko

Funder

Japan Society for the Promotion of Science

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Geology

Link

http://link.springer.com/article/10.1186/s40623-017-0736-x/fulltext.html

Reference29 articles.

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3. Carlson RW et al (1993) Variations in Venus cloud particle properties: a new view of Venus’s cloud morphology as observed by the Galileo near-infrared mapping spectrometer. Planet Space Sci 41:477–485

4. Drossart P et al (2007) A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express. Nature 450:641–645

5. Fukuhara T et al (2017) Large stationary gravity wave in the atmosphere of Venus. Nat Geosci 10:85–88. https://doi.org/10.1038/ngeo2873

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