- Abstract:
-
In its decade of operation the Cassini mission has allowed us to look deep into Saturn’s atmosphere and investigate the processes occurring below its enshrouding haze. We use Visual and Infrared Mapping Spectrometer (VIMS) 4.6—5.2 µm data from early in the mission to investigate the location and properties of Saturn’s cloud structure between 0.6 and 5 bars. We average nightside spectra from 2006 over latitude circles and model the spectral limb darkening using the NEMESIS radiative transfer a...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Accepted manuscript
- Files:
-
-
(pdf, 3.1MB)
-
- Publisher copy:
- 10.1016/j.icarus.2016.01.013
-
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- Publisher:
- Elsevier Publisher's website
- Journal:
- Icarus Journal website
- Volume:
- 271
- Pages:
- 400-417
- Publication date:
- 2016-01-19
- DOI:
- ISSN:
-
0019-1035
- URN:
-
uuid:08086a51-9a23-4bb4-b9d6-2ba30837369f
- Source identifiers:
-
584310
- Local pid:
- pubs:584310
- Copyright holder:
- Elseiver
- Copyright date:
- 2016
- Notes:
- © 2016 Published by Elsevier Inc. This is the accepted manuscript version of the article. The final version is available online from Elsevier at [10.1016/j.icarus.2016.01.013].
Journal article
Probing Saturn's tropospheric cloud with Cassini/VIMS
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