- Abstract:
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We review our current knowledge of the atmospheric dynamics of Venus prior to the Akatsuki mission, in the altitude range from the surface to approximately the cloud tops located at about 100 km altitude. The three-dimensional structure of the wind field in this region has been determined with a variety of techniques over a broad range of spatial and temporal scales (from the mesoscale to planetary, from days to years, in daytime and nighttime), spanning a period of about 50 years (from the 1...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted Manuscript
- Files:
-
-
(pdf, 4.6MB)
-
- Publisher copy:
- 10.1007/s11214-017-0389-x
-
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- Publisher:
- Springer Verlag Publisher's website
- Journal:
- Space Science Reviews Journal website
- Volume:
- 212
- Issue:
- 3-4
- Pages:
- 1541–1616
- Publication date:
- 2017-08-01
- Acceptance date:
- 2017-06-07
- DOI:
- EISSN:
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1572-9672
- ISSN:
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0038-6308
- Pubs id:
-
pubs:927424
- URN:
-
uri:536444dc-082e-4fa5-9949-0bc74e908774
- UUID:
-
uuid:536444dc-082e-4fa5-9949-0bc74e908774
- Local pid:
- pubs:927424
- Keywords:
- Copyright holder:
- Springer Science+Business Media B.V.
- Copyright date:
- 2017
- Notes:
-
© Springer Science+Business Media B.V. 2017. This is the accepted manuscript version of the article. The final version is available online from Springer Verlag at:
10.1007/s11214-017-0389-x
Journal article
The atmospheric dynamics of Venus
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