Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26444
Title: | The challenge and scientific application of the CO2 4.3 um atmospheric limb emission of Mars | Authors: | Lopez-Valverde, M. A. Piccialli, A. GIURANNA, MARCO Funke, B. López-Puertas, M. Jurado-Navarro, A. A. García-Comas, M. González-Galindo, F. López-Moreno, J. J. Jiménez-Monferrer, S. |
Issue Date: | 2015 | Volume: | European Planetary Science Congress 2015 (EPSC) | First Page: | EPSC2015-663 | Abstract: | The atmospheric fluorescent emissions of CO2 at 4.3- um have been observed in the daytime upper atmosphere of Mars from a limb geometry by the instruments OMEGA and PFS on board Mars Express [1, 8]. Initial analysis using non-local thermodynamic equilibrium (NLTE) models show that the emissions are well understood [7, 3, 6]. Yet they have not been exploited to derive important thermospheric parameters, like CO2 densities and temperatures. Our major goals are to improve current NLTE models with a joint study of OMEGA and PFS data, and to build an ambitious state-of-the-art NLTE retreival scheme for Mars. Recent progress has been made in these directions on Mars, Venus and Earth. We will present a summary of these efforts and the difficulties and expectatives for its application to the Mars Express data | Conference Name: | European Planetary Science Congress 2015 (EPSC) | Conference Place: | La Cité des Congrès, Nantes, France | Conference Date: | 27 settembre - 2 ottobre, 2015 | URI: | http://hdl.handle.net/20.500.12386/26444 | URL: | https://www.epsc2015.eu/ | Bibcode ADS: | 2015EPSC...10..663L | Fulltext: | open |
Appears in Collections: | 3.02 Abstract in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
EPSC2015-663-1.pdf | Abstract | 84.53 kB | Adobe PDF | View/Open |
Page view(s)
96
checked on Sep 12, 2024
Download(s)
22
checked on Sep 12, 2024
Google ScholarTM
Check
Items in DSpace are published in Open Access, unless otherwise indicated.