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Analysis of thermal emission from the nightside of Venus at 1.51 and 1.55 μm

Abstract:

We present radiative transfer modelling of thermal emission from the nightside of Venus in two ‘spectral window’ regions at 1.51 and 1.55 μm. The first discovery of these windows, reported by Erard et al. [Erard, S., Drossart, P., Piccioni, G., 2009. J. Geophys. Res. Planets 114, doi:10.1029/2008JE003116. E00B27], was achieved using a principal component analysis of data from the VIRTIS instrument on Venus Expr...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.icarus.2009.03.010

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Oxford college:
St Anne's College
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Oxford college:
Jesus College
Role:
Author
Publisher:
Elsevier
Journal:
Icarus More from this journal
Volume:
201
Issue:
2
Pages:
814-817
Publication date:
2009-03-18
Acceptance date:
2009-03-07
DOI:
EISSN:
1090-2643
ISSN:
0019-1035
Keywords:
Pubs id:
pubs:115551
UUID:
uuid:cb5708bc-d4af-44bf-854a-2dcb8b4af4fd
Local pid:
pubs:115551
Source identifiers:
115551
Deposit date:
2017-05-10

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