Article (Scientific journals)
MAVEN‐IUVS observations of the CO2+ UV doublet and CO Cameron bands in the Martian thermosphere: Aeronomy, seasonal and latitudinal distribution.
Gérard, Jean-Claude; Gkouvelis, Leonardos; Ritter, Birgit et al.
2019In Journal of Geophysical Research. Space Physics, 124, p. 5816-5827
Peer Reviewed verified by ORBi
 

Files


Full Text
Gerard_et_al-2019-Journal_of_Geophysical_Research__Space_Physics-2.pdf
Publisher postprint (1.37 MB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
Mars; ultraviolet dayglow; Cameron bands; CO2+ UV doublet; seasonal variation; model simulations; dust storm; composition
Abstract :
[en] We analyze two Martian years of dayglow measurements of the CO Cameron bands and the CO2+ ultraviolet doublet (UVD) at 298-299 nm with the Imaging UltraViolet Spectrograph on board the Maven orbiter. We show that the altitude and the brightness of the two emissions peaks are strongly correlated, although data were collected over a wide range of latitudes and seasons. veraged limb profiles are presented and compared with numerical simulations based on updated calculations of the production of the CO (a3Π) and the CO2+ (B 2Σ) states. The model simulations use the solar flux directly measured on board MAVEN with the Extreme Ultraviolet Monitor (EUVM) and the neutral densities provided by the Mars Climate Database (MCD) version 5.3, adapted to the conditions of the observations. We show that the altitude and the shape of the sample limb profiles are well reproduced using the MCD neutral atmosphere. The simulated peak intensities of the CO2+ UVD and Cameron bands are in good agreement considering the uncertainties on the excitation cross sections and the calibration of the IUVS and EUVM instruments. No significant adjustment of the electron impact cross section on CO2 to produce the a3Π state is needed. Seasonal-latitudinal maps of the Cameron and UVD peak altitude observed during two Martian years show variations as large as 23 km. Model simulations of the amplitude of these changes are in fair agreement with the observations except during the southern summer dust period (Ls = 270°-320°) when the calculated rise of the dayglow layer is underestimated.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Gérard, Jean-Claude  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO)
Gkouvelis, Leonardos ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
Ritter, Birgit ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
Hubert, Benoît  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
Jain, S.K.
Schnieder, N.M.
Language :
English
Title :
MAVEN‐IUVS observations of the CO2+ UV doublet and CO Cameron bands in the Martian thermosphere: Aeronomy, seasonal and latitudinal distribution.
Publication date :
June 2019
Journal title :
Journal of Geophysical Research. Space Physics
ISSN :
2169-9380
eISSN :
2169-9402
Publisher :
Wiley, Hoboken, United States - New Jersey
Volume :
124
Pages :
5816-5827
Peer reviewed :
Peer Reviewed verified by ORBi
Funders :
BELSPO - Politique scientifique fédérale
F.R.S.-FNRS - Fonds de la Recherche Scientifique
ASE - Agence Spatiale Européenne
Available on ORBi :
since 25 June 2019

Statistics


Number of views
74 (10 by ULiège)
Number of downloads
181 (12 by ULiège)

Scopus citations®
 
21
Scopus citations®
without self-citations
8
OpenCitations
 
15
OpenAlex citations
 
20

Bibliography


Similar publications



Contact ORBi