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Proceedings Paper

Venus atmospheric and surface studies from VIRTIS on Venus Express
Author(s): Gabriele E. Arnold; Pierre Drossart; Giuseppe Piccioni; Rainer Haus
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Paper Abstract

The Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on Venus Express, after five years in a polar Venus orbit, provided an enormous amount of new data including a three-dimensional view of the atmosphere and information on global surface properties of the planet. VIRTIS is a complex imaging spectrometer that combines three unique data channels in one compact instrument. Two of the channels are committed to spectral mapping (VIRTIS-M) and a third one to high spectral resolution studies (VIRTIS-H). The paper gives an overview about the experimental goals and the instrument performance. It discusses some selected scientific results achieved by VIRTIS, among them thermal structure and properties of the lower, middle and upper atmosphere including dynamics, polar vortex, nightglows, and NLTE effects as well as surface features obtained from nightside emission measurements in the NIR atmospheric windows.

Paper Details

Date Published: 16 September 2011
PDF: 17 pages
Proc. SPIE 8154, Infrared Remote Sensing and Instrumentation XIX, 81540W (16 September 2011); doi: 10.1117/12.892895
Show Author Affiliations
Gabriele E. Arnold, Deutsches Zentrum für Luft- und Raumfahrt e.V. (Germany)
Pierre Drossart, Lab. d'Études Spatiales et d'Instrumentation en Astrophysique, CNRS, Observatoire de Paris (France)
Giuseppe Piccioni, Istituto di Astrofisica Spaziale e Fisica Cosmica (Italy)
Rainer Haus, Westfälische Wilhelms-Univ. Münster (Germany)


Published in SPIE Proceedings Vol. 8154:
Infrared Remote Sensing and Instrumentation XIX
Marija Strojnik; Gonzalo Paez, Editor(s)

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