Brightness modulations of our nearest terrestrial planet Venus reveal atmospheric super-rotation rather than surface features.

Lee, Y J; García Muñoz, A; Imamura, T; Yamada, M; Satoh, T; Yamazaki, A; Watanabe, S

Lee, Y J; García Muñoz, A; Imamura, T; Yamada, M; Satoh, T; Yamazaki, A; Watanabe, S.

Afiliação

Lee YJ; Technische Universität Berlin, Berlin, Germany. y.j.lee@astro.physik.tu-berlin.de.
García Muñoz A; Technische Universität Berlin, Berlin, Germany.
Imamura T; GSFS, Univ. of Tokyo, Kashiwa, Japan.
Yamada M; Planetary Exploration Research Center (PERC), Narashino, Japan.
Satoh T; Institute of Space and Astronautical Science (ISAS/JAXA), Sagamihara, Japan.
Yamazaki A; Institute of Space and Astronautical Science (ISAS/JAXA), Sagamihara, Japan.
Watanabe S; Graduate School of Science, Univ. of Tokyo, Tokyo, Japan.

Nat Commun ; 11(1): 5720, 2020 11 12.

Article em En | MEDLINE | ID: mdl-33184258

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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nat Commun Assunto da revista: BIOLOGIA / CIENCIA Ano de publicação: 2020 Tipo de documento: Article País de afiliação: Alemanha

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