New observations of molecular nitrogen in the Martian upper atmosphere by IUVS on MAVEN - Faculté des Sciences de Sorbonne Université Accéder directement au contenu
Article Dans Une Revue Geophysical Research Letters Année : 2015

New observations of molecular nitrogen in the Martian upper atmosphere by IUVS on MAVEN

Michael H. Stevens
  • Fonction : Auteur
  • PersonId : 973563
Franck Lefèvre
Franck Montmessin

Résumé

We identify molecular nitrogen (N2) emissions in the Martian upper atmosphere using the Imaging Ultraviolet Spectrograph (IUVS) on NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. We report the first observations of the N2 Lyman-Birge-Hopfield (LBH) bands at Mars and confirm the tentative identification of the N2 Vegard-Kaplan (VK) bands. We retrieve N2 density profiles from the VK limb emissions and compare calculated limb radiances between 90 and 210 km against both observations and predictions from a Mars general circulation model (GCM). Contrary to earlier analyses using other satellite data, we find that N2 abundances exceed GCM results by about a factor of 2 at 130 km but are in agreement at 150 km. The analysis and interpretation are enabled by a linear regression method used to extract components of UV spectra from IUVS limb observations.
Fichier principal
Vignette du fichier
2015GL065319.pdf (535.76 Ko) Télécharger le fichier
Origine : Fichiers éditeurs autorisés sur une archive ouverte
Loading...

Dates et versions

insu-01238173 , version 1 (03-08-2020)

Identifiants

Citer

Michael H. Stevens, J. S. Evans, Nick M. Schneider, A. Ian F. Stewart, Justin Deighan, et al.. New observations of molecular nitrogen in the Martian upper atmosphere by IUVS on MAVEN. Geophysical Research Letters, 2015, 42 (21), pp.9050-9056. ⟨10.1002/2015GL065319⟩. ⟨insu-01238173⟩
122 Consultations
43 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More