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The formation of molecular hydrogen from water ice in the lunar regolith by energetic charged particles

Author
JORDAN, A. P1 ; STUBBS, T. J2 ; JOYCE, C. J1 ; SCHWADRON, N. A1 ; SPENCE, H. E1 ; WILSON, J. K1
[1] Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, New Hampshire, United States
[2] NASA Goddard Space Flight Center, Greenbelt, Maryland, United States
Source

Journal of geophysical research. Planets. 2013, Vol 118, Num 6, pp 1257-1264, 8 p ; ref : 1 p

ISSNNV
2169-9097
Scientific domain
Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
Publisher
Wiley, Hoboken, NJ
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Cratère lunaire Dissociation moléculaire Débit dose Fluorescence Glace Imagerie UV Lumière solaire Lune Molécule d'hydrogène Particule chargée Particule relativiste Particule solaire Profondeur pénétration Rayonnement cosmique galactique Rayonnement cosmique Régolithe Surface lunaire Vapeur eau Zone ombre Sonde spatiale LRO
Keyword (en)
Lunar crater Molecular dissociation Dose rates Fluorescence Ice Ultraviolet imaging Sunlight Moon Hydrogen molecules Charged particles Relativistic particle Solar particles Penetration depth Galactic cosmic rays Cosmic radiation Regolith Lunar surface Steam Shadow region LRO space probe
Keyword (es)
Cráter lunar Disociación molecular Imagenería UV Partícula relativista Zona sombra
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B20 Moon / 001E03B20D Features, landmarks, mineralogy, petrology, and atmosphere

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B50 Interplanetary space / 001E03B50E Solar wind interactions with planets, satellites, and comets

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
27667926

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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