Venus looks different from day to night across wavelengths: morphology from Akatsuki multispectral images

Abstract Since insertion into orbit on December 7, 2015, the Akatsuki orbiter has returned global images of Venus from its four imaging cameras at eleven discrete wavelengths from ultraviolet (283 and 365 nm) and near infrared (0.9–2.3 µm), to the thermal infrared (8–12 µm) from a near-equatorial or...

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Bibliografiset tiedot
Päätekijät: Sanjay S. Limaye, Shigeto Watanabe, Atsushi Yamazaki, Manabu Yamada, Takehiko Satoh, Takao M. Sato, Masato Nakamura, Makoto Taguchi, Tetsuya Fukuhara, Takeshi Imamura, Toru Kouyama, Yeon Joo Lee, Takeshi Horinouchi, Javier Peralta, Naomoto Iwagami, George L. Hashimoto, Seiko Takagi, Shoko Ohtsuki, Shin-ya Murakami, Yukio Yamamoto, Kazunori Ogohara, Hiroki Ando, Ko-ichiro Sugiyama, Nobuaki Ishii, Takumi Abe, Chikako Hirose, Makoto Suzuki, Naru Hirata, Eliot F. Young, Adriana C. Ocampo
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: SpringerOpen 2018-02-01
Sarja:Earth, Planets and Space
Aiheet:
Venus clouds
Morphology
Day
Night
Ultraviolet
Near infrared
Linkit:http://link.springer.com/article/10.1186/s40623-018-0789-5
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