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Mars odyssey neutron sensing of the south residual polar cap

Author
TOKAR, R. L1 ; ELPHIC, R. C1 ; FELDMAN, W. C1 ; FUNSTEN, H. O2 ; MOORE, K. R1 ; PRETTYMAN, T. H1 ; WIENS, R. C1
[1] Space and Atmospheric Sciences, Los Alamos National Laboratory, Los Alamos, New Mexico, United States
[2] Center for Space Science and Exploration, Los Alamos National Laboratory, Los Alamos, New Mexico, United States
Source

Geophysical research letters. 2003, Vol 30, Num 13, pp 10.1-10.4 ; ref : 16 ref

CODEN
GPRLAJ
ISSN
0094-8276
Scientific domain
Astronomy earth cosmic environment; Geophysics; Climatology, meteorology; Oceanography
Publisher
American Geophysical Union, Washington, DC
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Atmosphère planétaire Calotte polaire Carbone dioxyde Concentration Eau Glace Masse Modèle Phase solide Planète Mars Poussière atmosphérique Retombée poussière Spectrométrie neutron Vitesse dépôt
Keyword (en)
Planetary atmospheres Polar cap Carbon dioxide Concentration Water Ice Mass Models Solid phase Mars planet Atmospheric dust Dust fall out Neutron spectroscopy Deposition rate
Keyword (es)
Modelo Polvo atmosférico Recaída polvo Velocidad deposición
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B30 Planets, their satellites and rings. Asteroids / 001E03B30G Mars

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B35 Planetary, asteroid, and satellite characteristics and properties / 001E03B35G Surface features, cratering, and topography

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
15038204

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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