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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
Version:
Accepted manuscript

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Publisher copy:
10.1016/j.icarus.2016.04.022

Authors


Pérez-Hoyos, S More by this author
Sanz-Requena, JF More by this author
Sánchez-Lavega, A More by this author
More by this author
Department:
Oxford, MPLS, Physics, Atmos Ocean & Planet Physics
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Department:
Oxford, MPLS, Physics, Atmos Ocean & Planet Physics
MICIIN Project More from this funder
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Grant:
AYA2012-36666/
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Grant:
Programa Nacional de Movilidad de Recursos Humanos del Plan Nacional de I-D+i 2008-2011
Publisher:
Elsevier Publisher's website
Journal:
Icarus Journal website
Volume:
277
Pages:
1-18
Publication date:
2016-04-30
Acceptance date:
2016-04-14
DOI:
EISSN:
0019-1035
ISSN:
1090-2643
Pubs id:
pubs:623803
URN:
uri:dcc158d6-8173-4281-a4dc-d1bc9484d698
UUID:
uuid:dcc158d6-8173-4281-a4dc-d1bc9484d698
Local pid:
pubs:623803

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