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The atmospheric dynamics of Venus

Abstract:

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...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Accepted Manuscript

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Publisher copy:
10.1007/s11214-017-0389-x

Authors


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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Atmos Ocean & Planet Physics
Oxford college:
Trinity College
Role:
Author
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:
1572-9672
ISSN:
0038-6308
Pubs id:
pubs:927424
URN:
uri:536444dc-082e-4fa5-9949-0bc74e908774
UUID:
uuid:536444dc-082e-4fa5-9949-0bc74e908774
Local pid:
pubs:927424

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