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| Titel |
Synergetic investigation of CO on Mars and validation using PFS and CRISM observations |
| VerfasserIn |
Séverine Robert, Ann Carine Vandaele, Lori Neary, Frank Daerden, Evelyn De Wachter, Martine De Mazière, Giuseppe Sindoni, Marco Giuranna, Shohei Aoki, Michael D. Smith, Anne Grete Straume, Olivier Witasse, Carine Petit, Claude Camy-Peyret |
| Konferenz |
EGU General Assembly 2014
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| Medientyp |
Artikel
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| Sprache |
Englisch
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| Digitales Dokument |
PDF |
| Erschienen |
In: GRA - Volume 16 (2014) |
| Datensatznummer |
250097968
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| Publikation (Nr.) |
 EGU/EGU2014-13599.pdf |
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| Zusammenfassung |
| In the framework of the ESA General Studies Programme activity SIROCCO (Synergetic
SWIR and IR retrievals of near-surface concentrations of CH4 and CO for Earth and
Mars) and in preparation of the ExoMars TGO mission (2016), synergies between
different instruments onboard the TGO orbiter are investigated. The challenge is
to better capture CO information as close as possible to the surface, in view of
better addressing the understanding, quantification or monitoring of sources and
sinks.
ASIMUT-ALVL, a line-by-line radiative transfer code developed at IASB-BIRA
1, is
used to simulate spectra in the infrared range (0.7 – 4.5 μm) under instrumental
conditions corresponding to the instruments which will be onboard ExoMars TGO 2016.
Simulations were performed under various atmospheric conditions given by GEM-Mars
2 and
used for a sensitivity study of the different parameters involved (absorption lines selected,
CO concentration, etc).
We test synergetic approaches to combine different spectral domains and different
geometries (solar occultation and nadir). This seems necessary for an optimal exploitation of
near surface information from the available data. A synthetic dataset of spectra was created
for various scenarios. Different parameters were chosen to get a statistical and representative
set of spectra. Then retrievals were performed in non-synergetic and synergetic strategies.
The results of the fitting procedure and the benefits of the synergies will be discussed in this
communication.
In order to define a validation dataset, we used the results of the
Planetary Fourier Spectrometer (PFS) onboard Mars Express (MEX)
3 and
Compact Reconnaissance Imaging Spectrometer (CRISM) onboard Mars Reconnaissance Orbiter
(MRO) 4.
Seasonal trends of the two datasets were investigated for co-located observations. The data
considered in this study were collected from Ls =131, MY28 to Ls =103, MY31. CO
mixing ratios from PFS will be retrieved, under synergetic and non-synergetic conditions, and
then compared to the CRISM values. |
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