http://www.cnr.it/ontology/cnr/individuo/prodotto/ID276868
Cloud-top temporal variation of Saturn's 2011-2012 stratospheric vortex by means of Cassini/VIMS-V data analysis (Abstract/Poster in atti di convegno)
- Type
- Label
- Cloud-top temporal variation of Saturn's 2011-2012 stratospheric vortex by means of Cassini/VIMS-V data analysis (Abstract/Poster in atti di convegno) (literal)
- Anno
- 2013-01-01T00:00:00+01:00 (literal)
- Alternative label
F. Oliva (1), A. Adriani (1), G.L. Liberti (2), M. L. Moriconi (2) (2013)
Cloud-top temporal variation of Saturn's 2011-2012 stratospheric vortex by means of Cassini/VIMS-V data analysis
in European Planetary Science Congress 2013, London,UK, 8-13 settembre 2013
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- F. Oliva (1), A. Adriani (1), G.L. Liberti (2), M. L. Moriconi (2) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#volumeInCollana
- Note
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- (1) INAF-IAPS, Rome, Italy
(2) CNR-ISAC, Rome, Italy (literal)
- Titolo
- Cloud-top temporal variation of Saturn's 2011-2012 stratospheric vortex by means of Cassini/VIMS-V data analysis (literal)
- Abstract
- In this work, selected regions of the giant vortex
observed at Saturn since January 2011, have been
investigated by analyzing the observations from the
visual channel of the Visual and Infrared Mapping
Spectrometer (VIMS-V) on board the Cassini
spacecraft. Previously, a forward radiative transfer
model has been developed, based on the LibRadtran
code [13], adapted to the atmosphere of Saturn. Then
an inverse code, based on the optimal estimation
technique [14], has been implemented to retrieve the
microphysical and geometrical properties of the
clouds. Best fits of the radiance spectra relative to the
vortex are produced and then the cloud top pressures
are estimated. Data retrieved on a time lapse of
months allow to investigate the temporal variation of
the vortex's cloud properties. (literal)
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