Distribution of HCN in Titan’s upper atmosphere from Cassini/VIMS observations at 3 um

Autor: A. Adriani1, B.M. Dinelli2, M. López-Puertas3, M. García-Comas3, M.L. Moriconi4, E. D’Aversa1, B. Funke3, A. Coradini1

Publikováno v: Icarus (N.Y.N.Y. 1962) 214 (2011).
info:cnr-pdr/source/autori:A. Adriani1, B.M. Dinelli2, M. López-Puertas3, M. García-Comas3, M.L. Moriconi4, E. D’Aversa1, B. Funke3, A. Coradini1/titolo:Distribution of HCN in Titan’s upper atmosphere from Cassini%2FVIMS observations at 3 um/doi:/rivista:Icarus (N.Y.N.Y. 1962)/anno:2011/pagina_da:/pagina_a:/intervallo_pagine:/volume:214

Cassini/VIMS limb observations have been used to retrieve vertical profiles of hydrogen cyanide (HCN) from its 3 lm emission in the region from 600 to 1100 km altitude at daytime. While the daytime emission is large up to about 1100 km, it vanishes a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::2799b96ae1f6c3671440c9109e2816d9
http://www.cnr.it/prodotto/i/45140

A Radiative Transfer model for the atmospheres of the Outer Planets

Autor: Colosimo, S. F.1, A. Adriani1, M.L. Moriconi2, B.M. Dinelli 3, J.I. Lunine1, E. D’aversa1, A. Coradini 1, D. Grassi1

Publikováno v: EGU, Vienna, 2008
info:cnr-pdr/source/autori:Colosimo, S. F.1, A. Adriani1, M.L. Moriconi2, B.M. Dinelli 3, J.I. Lunine1, E. D’aversa1, A. Coradini 1, D. Grassi1/congresso_nome:EGU/congresso_luogo:Vienna/congresso_data:2008/anno:2008/pagina_da:/pagina_a:/intervallo_pagine

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::0e4d54c22cfdf847ef94e16006a21616
http://www.cnr.it/prodotto/i/121306