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

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).
Type de document :
Communication dans un congrès
sixth international workshop on the Mars atmosphere: Modelling and observations, Jan 2017, Granada, Spain
Liste complète des métadonnées

Littérature citée [5 références]  Voir  Masquer  Télécharger

https://hal-insu.archives-ouvertes.fr/insu-01451113
Contributeur : Catherine Cardon <>
Soumis le : mardi 31 janvier 2017 - 16:26:43
Dernière modification le : mardi 29 mai 2018 - 12:51:05
Document(s) archivé(s) le : lundi 1 mai 2017 - 16:02:45

Fichier

schneider_granada2017.pdf
Fichiers produits par l'(les) auteur(s)

Identifiants

  • HAL Id : insu-01451113, version 1

Collections

Citation

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〉

Partager

Métriques

Consultations de la notice

283

Téléchargements de fichiers

64