Titan's ground reflectance retrieval from Cassini-VIMS data taken during the July 2nd, 2004 fly-by at 2 AM UT (Articolo in rivista)

Type

• Articolo in rivista (Classe)
• Prodotto della ricerca (Classe)

Label

• Titan's ground reflectance retrieval from Cassini-VIMS data taken during the July 2nd, 2004 fly-by at 2 AM UT (Articolo in rivista) (literal)

Anno

• 2005-01-01T00:00:00+01:00 (literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi

• 10.1007/s11038-005-9057-3 (literal)

Alternative label

• A. Adriani (a); A. Gardini (a); E. D'Aversa (a); A. Coradini (a); M. L. Moriconi (b); G. L. Liberti (b); R. Orosei (c); G. Filacchione (c) (2005)
  Titan's ground reflectance retrieval from Cassini-VIMS data taken during the July 2nd, 2004 fly-by at 2 AM UT
  in Earth, moon, and planets
  (literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori

• A. Adriani (a); A. Gardini (a); E. D'Aversa (a); A. Coradini (a); M. L. Moriconi (b); G. L. Liberti (b); R. Orosei (c); G. Filacchione (c) (literal)

Pagina inizio

• 109 (literal)

Pagina fine

• 117 (literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume

• 96 (literal)

Rivista

• Earth, moon, and planets (Rivista)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroFascicolo

• 3-4 (literal)

Note

• ISI Web of Science (WOS) (literal)
• Scopu (literal)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni

• (a) INAF, Istituto di Fisica dello Spazio Interplanetario, Roma, Italy (b) CNR, Istituto di Scienza dell'Atmosfera e del Clima, Roma, Italy (c) INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica, Roma, Italy (literal)

Titolo

• Titan's ground reflectance retrieval from Cassini-VIMS data taken during the July 2nd, 2004 fly-by at 2 AM UT (literal)

Abstract

• An attempt to evaluate the preliminary values of the Titan's surface albedo at 2 ìm from the first Cassini-VIMS observations of the moon is presented. The methodology is based on the application of radiative transfer calculations and a microphysical model of the Titan atmosphere based on fractal aerosol. As a first guess, the surface has been considered flat and lambertian. The results are presented as a function of the geographical coordinates associated to the image pixels. The libRadtran package, using the radiative transfer equation solver DISORT 2.0, has been applied for the calculations. A test run to evaluate the model performances, using ground based observations of Titan as reference in the range of wavelengths 0.3-1.0 ìm, has been carried out.The retrieved values of the surface albedo range between 0.03 and 0.22. (literal)

Prodotto di

• Institute of atmospheric sciences and climate (ISAC) (Istituto)

Autore CNR

• MARIA LUISA MORICONI (Unità di personale interno)
• GIAN LUIGI LIBERTI (Unità di personale interno)

Incoming links:

Prodotto

• Institute of atmospheric sciences and climate (ISAC) (Istituto)

Autore CNR di

• MARIA LUISA MORICONI (Unità di personale interno)
• GIAN LUIGI LIBERTI (Unità di personale interno)

Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#rivistaDi

• Earth, moon, and planets (Rivista)