http://www.cnr.it/ontology/cnr/individuo/prodotto/ID191885
Model validation of the polar clouds at Saturn as inferred by Cassini/VIMS data in the visual range (Abstract/Poster in convegno)
- Type
- Label
- Model validation of the polar clouds at Saturn as inferred by Cassini/VIMS data in the visual range (Abstract/Poster in convegno) (literal)
- Anno
- 2012-01-01T00:00:00+01:00 (literal)
- Alternative label
F. Oliva , A. Adriani , M. L. Moriconi , G. Liberti (2012)
Model validation of the polar clouds at Saturn as inferred by Cassini/VIMS data in the visual range
in European Planetary Science Congress 2012, Madrid, 23-28 September 2012
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- F. Oliva , A. Adriani , M. L. Moriconi , G. Liberti (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
- http://meetingorganizer.copernicus.org/EPSC2012/EPSC2012-549.pdf (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#volumeInCollana
- Vol. 7 EPSC2012-549 2012 (literal)
- Note
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- INAF-IAPS, Rome, Italy, CNR-ISAC, Rome, Italy (literal)
- Titolo
- Model validation of the polar clouds at Saturn as inferred by Cassini/VIMS data in the visual range (literal)
- Abstract
- In this study the microphysical, optical and
geometrical parameters obtained by Colosimo et al
[5] to represent the clouds observed in the South Pole
atmosphere of Saturn are used in a radiative transfer
model to simulate the corresponding observations
from Cassini/VIMS VIS-channel data in the
wavelength range 0.84-1 micron. The disagreement
between simulated and observed spectra has been
interpreted taking into account the different nature of
the measurements. Taking into account possible
sources of discrepancies, an adjustment of the model
parameters is suggested. The proposed values, reduce
the difference between the simulations and the
measurements from ~ 63% down to ~ 17%. (literal)
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- Autore CNR
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