Wind field estimation at 5.0 micron by Juno/JIRAM imaging of Jupiter's poles

Autor: M. L. Moriconi2, A. Adriani1, A. Mura1, A. Migliorini1, F. Altieri1, G. Filacchione1, B.M. Dinelli2, F. Tosi1, F. Fabiano3, G. Sindoni 1, D. Turrini1, R. Noschese1, A. Cicchetti1, G. Piccioni1, C. Plainaki4, A. Olivieri4, S. Bolton5, S. Atreya6, J. Lunine7

Publikováno v: EPSC, Riga, Lettonia, 17-22 September 2017
info:cnr-pdr/source/autori:M. L. Moriconi2, A. Adriani1, A. Mura1, A. Migliorini1, F. Altieri1, G. Filacchione1, B.M. Dinelli2, F. Tosi1, F. Fabiano3, G. Sindoni 1, D. Turrini1, R. Noschese1, A. Cicchetti1, G. Piccioni1, C. Plainaki4, A. Olivieri4, S. Bolton5, S. Atreya6, J. Lunine7/congresso_nome:EPSC/congresso_luogo:Riga, Lettonia/congresso_data:17-22 September 2017/anno:2017/pagina_da:/pagina_a:/intervallo_pagine

During the JP4 pass on Feb 2nd 2017 the Jovian InfraRed Auroral Mapper (JIRAM, [1]) got many observations of the two Jupiter's poles when the Juno spacecraft at perijove passed at very short distance from the planet. The spatial resolutions of the ac

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::1607aa40bd6a2b6a6eab4b165ba7d9ca
https://publications.cnr.it/doc/370682

CO concentration in the upper stratosphere and mesosphere of Titan: non-LTE analysis of VIMS dayside limb observations at 4.7 um

Autor: F. Fabiano1, 2, M. Lopez Puertas4, A. Adriani3, M.L. Moriconi3, E. D'Aversa3, M. Ridolfi1, B.M. Dinelli2

Publikováno v: XII Congresso Nazionale Scienze Planetarie, Bormio (SO),Italia, 2-6/02/2015
info:cnr-pdr/source/autori:F. Fabiano1,2, M. Lopez Puertas4, A. Adriani3, M.L. Moriconi3, E. D'Aversa3, M. Ridolfi1, and B.M. Dinelli2/congresso_nome:XII Congresso Nazionale Scienze Planetarie/congresso_luogo:Bormio (SO),Italia/congresso_data:2-6%2F02%2F2015/anno:2015/pagina_da:/pagina_a:/intervallo_pagine

During the last 20 years, many works have focused on the atmospheric concentration of CO on Titan, giving contradictory results. In particular, no measurement of the CO abundance above 300km has been done yet, due to the faint emission of CO above th

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::eec82931ac5d879dc91e7a5c5e36f80d
http://www.cnr.it/prodotto/i/319006

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