First Observation of the Oxygen 630 nm Emission in the Martian Dayglow

Author:

Gérard J.‐C.1ORCID,Aoki S.12ORCID,Gkouvelis L.13ORCID,Soret L.1ORCID,Willame Y.2,Thomas I. R.2ORCID,Depiesse C.2,Ristic B.2ORCID,Vandaele A. C.2,Hubert B.1,Daerden F.2ORCID,Patel M. R.4ORCID,López‐Moreno J.‐J.5,Bellucci G.6,Mason J. P.4,López‐Valverde M. A.5ORCID

Affiliation:

1. LPAP STAR Institute Université de Liège Belgium

2. Royal Belgian Institute for Space Aeronomy Brussels Belgium

3. NASA/Ames Research Center Moffet Field Mountain view CA USA

4. School of Physical Sciences The Open University Milton Keynes UK

5. Instituto de Astrofìsica de Andalucía/CSIC Granada Spain

6. Istituto di Astrofisica e Planetologia Spaziali INAF Rome Italy

Funder

European Space Agency

Belgian Federal Science Policy Office

Ministerio de Ciencia, Innovación y Universidades

UK Space Agency

Agenzia Spaziale Italiana

Hill, Holliday, Connors, Cosmopulos

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference34 articles.

1. The Atmosphere of Mars

2. Effective collision strengths for forbidden transitions in e-N and e-o scattering

3. Far‐ultraviolet spectroscopy of venus and mars at 4 A resolution with the Hopkins Ultraviolet Telescope on Astro‐2;Feldman P. D.;Acta Pathologica Japonica,2000

4. Improved general circulation models of the Martian atmosphere from the surface to above 80 km

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