Solar-wind control of the hot oxygen corona around Mars
- Author
- KANEDA, Kaori1 ; TERADA, Naoki2 3 ; MACHIDA, Shinobu1
[1] Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan
[2] Space Environment Group, Applied Electromagnetic Research Center, National Institute of Information and Communications Technology, Tokyo, Japan
[3] Core Research for Evolutional Science and Technology, Japan Science and Technology Agency, Saitama, Japan - Source
Journal of geophysical research. 2009, Vol 114, Num E2 ; E02007.1-E02007.11 ; ref : 3/4 p
- ISSN
- 0148-0227
- Scientific domain
- Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
- Publisher
- American Geophysical Union, Washington, DC
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Altitude Condition non stationnaire Couplage Cours eau Court terme Densité Exosphère Gaine magnétosphérique Ionosphère Modèle 1 dimension Modèle MHD Monde Méthode Monte Carlo Oxygène Planète Mars Plomb Pression dynamique Soleil Symétrie axiale Taux fuite Vent solaire
- Keyword (en)
- altitude Non stationary condition coupling streams Short term density Exosphere Magnetosheath ionosphere one-dimensional models MHD model global Monte Carlo analysis oxygen Mars lead Dynamic pressure Sun Axial symmetry Escape rate solar wind
- Keyword (es)
- Altitud Condición no estacionaria Curso agua Corto plazo Densidad Exósfera Vaina magnetosférica Ionosfera Modelo 1 dimensión Modelo MHD Mundo Oxígeno Planeta Marte Plomo Presión dinámica Sol Simetría axial Tasa fuga Viento solar
- Classification
- Discipline
- Earth sciences
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 21403497
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
10.1029/2008JE003234 
https://dx.doi.org/10.1029/2008JE003234
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