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Saturn's tropospheric particles phase function and spatial distribution from Cassini ISS 2010-11 observations

Abstract:

The phase function describes the way particles scatter the incoming radiation. This is a fundamental piece of knowledge in order to understand how a planetary atmosphere scatters sunlight and so it has a profound influence in the retrieved atmospheric properties such as cloud height, particle density distribution and radiative forcing by aerosols. In this work we analyze data from the Imaging Science Subsystem (ISS) instrument onboard Cassini spacecraft to determine the particle phase functio...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.icarus.2016.04.022

Authors


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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
Role:
Author
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Grant:
AYA2012-36666 with FEDER support
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Grant:
IT765-80913,
UPV/EHUUFI11/55
Publisher:
Elsevier
Journal:
Icarus More from this journal
Volume:
277
Pages:
1-18
Publication date:
2016-04-30
Acceptance date:
2016-04-14
DOI:
EISSN:
1090-2643
ISSN:
0019-1035
Keywords:
Pubs id:
pubs:623803
UUID:
uuid:ee836463-0aec-4ece-90a9-7619f3c40833
Local pid:
pubs:623803
Source identifiers:
623803
Deposit date:
2016-06-08

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