The lunar photoelectron sheath: A change in trapping efficiency during a solar storm
- Author
- FARRELL, W. M1 4 ; POPPE, A. R2 4 ; ZIMMERMAN, M. I1 3 4 ; HALEKAS, J. S2 4 ; DELORY, G. T2 4 ; KILLEN, R. M1 4
[1] NASA Goddard Space Flight Center, Greenbelt, Maryland, United States
[2] Space Sciences Laboratory, The University of California, Berkeley, Berkeley, California, United States
[3] Oak Ridge Associated Universities, Oak Ridge, Tennessee, United States
[4] NASA Lunar Science Institute, NASA Ames Research Center, Moffett Field, California, United States - Source
Journal of geophysical research. Planets. 2013, Vol 118, Num 5, pp 1114-1122, 9 p ; ref : 1/2 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)
- Ejection masse coronale Electron solaire Electron thermique Flux électrons Lune Méthode particule dans cellule Photoélectron Piégeage particule Plasma Potentiel équilibre Surface lunaire Vent solaire
- Keyword (en)
- Coronal mass ejection Solar electrons Thermal electron Electron flux Moon Particle in cell method Photoelectron Particle trapping Plasma Equilibrium potential Lunar surface Solar wind
- Keyword (es)
- Eyección masa coronal Electrón térmico Flujo electrones Método partícula dentro célula Fotoelectrón Captura partícula Potencial equilibrio
- 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
- 27667915
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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DOI
10.1002/jgre.20086 
https://dx.doi.org/10.1002/jgre.20086
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