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Algorithm for Extraction of Surface Emissivity in the Context of VIRTIS on Venus Express

Müller, N. und Helbert, J. und Hashimoto, G. und Marinangeli, L. und Piccioni, G. und Drossart, P. (2006) Algorithm for Extraction of Surface Emissivity in the Context of VIRTIS on Venus Express. In: Eos Trans. AGU Fall Meeting suppl., 87 (52), P42A-07. American Geophysical Union Fall Meeting 2006, 2006-12-11 - 2006-12-15, San Francisco (USA).

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Venus nightside multispectral images aquired by VIRTIS contain information of surface emissivity at wavelengths close to 1 micron. This information is relayed by thermal emissions of the surface escaping to space through the NIR spectral ‘windows' in the atmosphere. On its way through the atmosphere the thermal radiation is modified by scattering and absorption by clouds. Variations in the optical thickness of the clouds modulate the spatial distribution of upwelling radiation. Multiple reflections between surface and clouds generally wash out image contrast from surface emissivity. We present an algorithm to extract surface emissivities by separating atmospheric influences from the images inside the spectral windows at 1.02, 1.10 and 1.18 micron. The necessary processing steps detailed are: 1) Removal of scattered sunlight 2) Binning of appropriate images inside the window spectral ranges 3) Correction of limb darkening 4) Removal of contrast due to attenuation by clouds 5) Removal of contrast due to surface temperature 6) Correction for multiple cloud-surface-reflections For a first quick guess on general trends of emissivity with respect to geological circumstances this algorithm is applied with several simplifications and ad-hoc assumptions. This simple model assumes the atmosphere of Venus to be one horizontally homogenous layer with spatial variation of transmittance allowing for direct inversion of the data. For an improved estimation of surface emissivity tabulated results from previous forward modeling of radiative transfer are used for steps 2) to 6). With this approach the accuracy of a detailed modeling of the atmosphere of Venus is combined with the speed and traceability of the step-by-step inversion of radiance data using the simplified model.

Dokumentart:Konferenzbeitrag (NICHT SPEZIFIZIERT)
Titel: Algorithm for Extraction of Surface Emissivity in the Context of VIRTIS on Venus Express
AutorenInstitution oder E-Mail-AdresseAutoren-ORCID-iD
Hashimoto, G.Graduate School of Science and Technology, Kobe University, Nada-ku, Kobe, 657- 8501 JapanNICHT SPEZIFIZIERT
Marinangeli, L.IRSPS, Universita d Annunzio, Viale Pindaro, 42, Pescara, 65127 ItalyNICHT SPEZIFIZIERT
Piccioni, G.INAF - IASF Roma, Via del Fosso del Cavaliere 100, Roma, 00133NICHT SPEZIFIZIERT
Drossart, P.LESIA - Observatoire de Paris, 61 avenue de l observatoire, Paris, 75014 FranceNICHT SPEZIFIZIERT
Datum:Dezember 2006
Erschienen in:Eos Trans. AGU Fall Meeting suppl.
In Open Access:Nein
In ISI Web of Science:Nein
Name der Reihe:Eos Transactions AGU
Stichwörter:Remote sensing, Surface materials and properties, Extra-solar planets, Planetary volcanism
Veranstaltungstitel:American Geophysical Union Fall Meeting 2006
Veranstaltungsort:San Francisco (USA)
Veranstaltungsart:internationale Konferenz
Veranstaltungsdatum:2006-12-11 - 2006-12-15
Veranstalter :AGU
HGF - Forschungsbereich:Verkehr und Weltraum (alt)
HGF - Programm:Weltraum (alt)
HGF - Programmthema:W EW - Erforschung des Weltraums
DLR - Schwerpunkt:Weltraum
DLR - Forschungsgebiet:W EW - Erforschung des Weltraums
DLR - Teilgebiet (Projekt, Vorhaben):W - Vorhaben Vergleichende Planetologie (alt)
Standort: Berlin-Adlershof
Institute & Einrichtungen:Institut für Planetenforschung > Planetenphysik
Hinterlegt von: Musiol, Stefanie
Hinterlegt am:15 Jan 2007
Letzte Änderung:27 Apr 2009 13:25

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