Equatorial jet in the lower to middle cloud layer of Venus revealed by Akatsuki

The Venusian atmosphere is in a state of superrotation where prevailing westward winds move much faster than the planet’s rotation. Venus is covered with thick clouds that extend from about 45 to 70 km altitude, but thermal radiation emitted from the lower atmosphere and the surface on the planet’s...

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Detalles Bibliográficos
Autores principales: Horinouchi, Takeshi, Murakami, Shin-ya, Satoh, Takehiko, Peralta, Javier, Ogohara, Kazunori, Kouyama, Toru, Imamura, Takeshi, Kashimura, Hiroki, Limaye, Sanjay S., McGouldrick, Kevin, Nakamura, Masato, Sato, Takao M., Sugiyama, Ko-ichiro, Takagi, Masahiro, Watanabe, Shigeto, Yamada, Manabu, Yamazaki, Atsushi, Young, Eliot F.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: 2017
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5990972/
https://www.ncbi.nlm.nih.gov/pubmed/29887914
http://dx.doi.org/10.1038/ngeo3016

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5990972/
https://www.ncbi.nlm.nih.gov/pubmed/29887914
http://dx.doi.org/10.1038/ngeo3016

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