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

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 orbit. The...

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Detalles Bibliográficos
Autores principales: Limaye, Sanjay S., Watanabe, Shigeto, Yamazaki, Atsushi, Yamada, Manabu, Satoh, Takehiko, Sato, Takao M., Nakamura, Masato, Taguchi, Makoto, Fukuhara, Tetsuya, Imamura, Takeshi, Kouyama, Toru, Lee, Yeon Joo, Horinouchi, Takeshi, Peralta, Javier, Iwagami, Naomoto, Hashimoto, George L., Takagi, Seiko, Ohtsuki, Shoko, Murakami, Shin-ya, Yamamoto, Yukio, Ogohara, Kazunori, Ando, Hiroki, Sugiyama, Ko-ichiro, Ishii, Nobuaki, Abe, Takumi, Hirose, Chikako, Suzuki, Makoto, Hirata, Naru, Young, Eliot F., Ocampo, Adriana C.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2018
Materias:
Full Paper
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6954018/
https://www.ncbi.nlm.nih.gov/pubmed/31983884
http://dx.doi.org/10.1186/s40623-018-0789-5

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6954018/
https://www.ncbi.nlm.nih.gov/pubmed/31983884
http://dx.doi.org/10.1186/s40623-018-0789-5

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