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Multiple-wavelength sensing of Jupiter during the Juno mission's first perijove passage

Autor: G. S. Orton1, T. Momary1, A. P. Ingersoll2, A. Adriani3, C. J. Hansen4, M. Janssen1, J. Arballo1, S. K. Atreya4, S. Bolton5, S. Brown1, M. Caplinger6, D. Grassi3, C. Li1, S. Levin1, M. L. Moriconi3, 7, A. Mura3, G. Sindoni3

Publikováno v: Geophysical research letters (Online) (2017).
info:cnr-pdr/source/autori:G. S. Orton1, T. Momary1, A. P. Ingersoll2, A. Adriani3, C. J. Hansen4, M. Janssen1, J. Arballo1, S. K. Atreya4, S. Bolton5, S. Brown1, M. Caplinger6, D. Grassi3, C. Li1, S. Levin1, M. L. Moriconi3,7, A. Mura3, and G. Sindoni3/titolo:Multiple-wavelength sensing of Jupiter during the Juno mission's first perijove passage/doi:/rivista:Geophysical research letters (Online)/anno:2017/pagina_da:/pagina_a:/intervallo_pagine:/volume

We compare Jupiter observations made around 27 August 2016 by Juno's JunoCam, Jovian Infrared Auroral Mapper (JIRAM), MicroWave Radiometer (MWR) instruments, and NASA's Infrared Telescope Facility. Visibly dark regions are highly correlated with brig

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::4ff8487a5072fcc6cea1c2b9f6319ab2
http://www.cnr.it/prodotto/i/370841

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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

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Elevadas concentraciones de PAHs en la alta atmósfera de Titán

Autor: M. López-Puertas1, M. García-Comas1, B. Funke1, B.M. Dinelli2, A. Adriani3, M.L. Moriconi4, C. Boersma5 y L.J. Allamandola5

Publikováno v: III Encuentro sobre Ciencias Planetarias y Exploración del Sistema Solar, Madrid, 19-21 June 2013
info:cnr-pdr/source/autori:M. López-Puertas1, M. García-Comas1, B. Funke1, B.M. Dinelli2, A. Adriani3, M.L. Moriconi4, C. Boersma5 y L.J. Allamandola5 /congresso_nome:III Encuentro sobre Ciencias Planetarias y Exploración del Sistema Solar/congresso_luogo:Madrid/congresso_data:19-21 June 2013/anno:2013/pagina_da:/pagina_a:/intervallo_pagine

En este trabajo presentamos el análisis de las observaciones de la alta atmósfera de Titán en la región de 3.3 µ?m tomadas por el instrumento VIMS (Visual---Infrared Mapping Spectrometer) a bordo de la misión Cassini. En primer lugar presenta

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::dbc3fbe7b4e7b231444c7abd80f86661
http://www.cnr.it/prodotto/i/216467

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Large abundances of PAHs in Titan's Upper Atmosphere

Autor: Manuel López-Puertas1, B. Funke1, M. García-Comas1, B. Dinelli2, M. Moriconi2, A. Adriani3, E. D'Aversa3, L. Allamandola4, C. Boersma4

Publikováno v: 2nd National Conference on Laboratory and Molecular Astrophysics, Sevilla (Spain), November 14-16, 2012
info:cnr-pdr/source/autori:Manuel López-Puertas1, B. Funke1, M. García-Comas1,B. Dinelli2, M. Moriconi2,A. Adriani3, E. D'Aversa3,L. Allamandola4, C. Boersma4/congresso_nome:2nd National Conference on Laboratory and Molecular Astrophysics/congresso_luogo:Sevilla (Spain)/congresso_data:November 14-16, 2012/anno:2012/pagina_da:/pagina_a:/intervallo_pagine

In this paper we present the analysis of the Cassini/VIMS limb daytime observations of Titan upper atmosphere in the 3.3 um region. This spectral region is dominated by the strong CH4 bands. However, we have found that, in addition to CH4, there is a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::9dbb0124c7e17081cbfc12db46ea929e
http://www.cnr.it/prodotto/i/212910

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An unidentified emission in Titan's upper atmosphere

Autor: B.M. Dinelli1, M. López-Puertas2, A. Adriani3, M.L. Moriconi4, M. García-Comas2, B.Funke2, E. D'Aversa3, A. Coradini3

Publikováno v: EPSC-DPS Joint Meeting 2011, Nantes (FR), 2011
info:cnr-pdr/source/autori:B.M. Dinelli1, M. López-Puertas2, A. Adriani3, M.L. Moriconi4, M. García-Comas2, B.Funke2, E. D'Aversa3, and A. Coradini3/congresso_nome:EPSC-DPS Joint Meeting 2011/congresso_luogo:Nantes (FR)/congresso_data:2011/anno:2011/pagina_da:/pagina_a:/intervallo_pagine

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::c20ed8cc1fce8e552c298f19351c6e76
https://publications.cnr.it/doc/121553

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