Global UV Imaging by MAVEN/IUVS: Diurnal Cloud Formation, Dust Storms and Atmospheric Scattering

Nicholas M. Schneider 1 Justin I. Deighan 1 Sonal Kumar Jain 1 Alysa Derks 1 Michael S. Chaffin 1 Matteo Crismani 1 A. Ian F. Stewart 1 William E. Mcclintock 1 Gregory M. Holsclaw 1 Bruce M. Jakosky 1 Franck Lefèvre 2 Franck Montmessin 2 Michael J. Wolff 3 Arnaud Stiepen 4 Michael H. Stevens 5 J. Scott Evans 6 Roger V. Yelle 7 Daniel Y. Lo 7 John T. Clarke 8
1 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
2 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
3 SSI - Space Science Institute [Boulder]
4 LPAP - Laboratoire de Physique Atmosphérique et Planétaire
5 NRL - Naval Research Laboratory
6 Computational Physics, Inc.
7 LPL - Lunar and Planetary Laboratory [Tucson]
8 CSP - Center for Space Physics [Boston]
Abstract : A new UV spectral imaging dataset of Mars global images is being obtained by the Imaging Ul- traViolet Spectrograph (IUVS) on the Mars Atmos- phere and V olatile Evolution mission (MA VEN). Of particular interest for atmospheric studies are spec- trally-resolved mid-UV datacubes as shown in Fig- ure 1. Clouds, haze, dust and ozone can all be detect- ed and quantified through image analysis and re- trieval. IUVS observations are the only MAVEN data capable of probing below the spacecraft alti- tude, and provide an important link between the denser atmosphere and escape processes which are MAVEN’s primary focus (Jakosky et al. 2015).
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Nicholas M. Schneider, Justin I. Deighan, Sonal Kumar Jain, Alysa Derks, Michael S. Chaffin, et al.. Global UV Imaging by MAVEN/IUVS: Diurnal Cloud Formation, Dust Storms and Atmospheric Scattering. sixth international workshop on the Mars atmosphere: Modelling and observations, Jan 2017, Granada, Spain. ⟨insu-01451113⟩

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