Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation

We present distributions of the zonal-mean temperature and static stability in the Venusian atmosphere obtained from Venus Express and Akatsuki radio occultation profiles penetrating down to an altitude of 40 km. At latitudes equatorward of 75°, static stability derived from the observed temperature...

Descripción completa

Detalles Bibliográficos
Autores principales: Ando, Hiroki, Imamura, Takeshi, Tellmann, Silvia, Pätzold, Martin, Häusler, Bernd, Sugimoto, Norihiko, Takagi, Masahiro, Sagawa, Hideo, Limaye, Sanjay, Matsuda, Yoshihisa, Choudhary, Raj Kumar, Antonita, Maria
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2020
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7044293/
https://www.ncbi.nlm.nih.gov/pubmed/32103048
http://dx.doi.org/10.1038/s41598-020-59278-8

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7044293/
https://www.ncbi.nlm.nih.gov/pubmed/32103048
http://dx.doi.org/10.1038/s41598-020-59278-8

Ejemplares similares