Role of magnetic reconnection in Venus ionopause activity
- Autor
- DREHER, J1 ; BIRK, G. T1 ; SCHINDLER, K1 ; OTTO, A
[1] Ruhr-Univ. Bochum, Theoretische Physik IV, 44780 Bochum, Germany - Fuente
Journal of geophysical research. 1995, Vol 100, Num A8, pp 14833-14841 ; ref : 17 ref
- ISSN
- 0148-0227
- Campo Científico
- Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
- Editor
- American Geophysical Union, Washington, DC
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- English
- Palabra clave (fr)
- Atmosphère planétaire Corde flux Instabilité déchirure Ionosphère planétaire Magnétohydrodynamique Planète Vénus Reconnexion magnétique Simulation numérique Vent solaire
- Palabra clave (in)
- Planetary atmospheres Flux rope Tearing instability Planetary ionospheres Magnetohydrodynamics Venus planet Magnetic reconnection Numerical simulation Solar wind
- Palabra clave (es)
- Cuerda flujo Simulación numérica
- Clasificación
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B30 Planets, their satellites and rings. Asteroids / 001E03B30E Venus
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B35 Planetary, asteroid, and satellite characteristics and properties / 001E03B35K Ionospheres; magnetospheres
- 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
- Disciplina
- Astronomy
- Procedencia
- Inist-CNRS
- Base de datos
- PASCAL
- Identificador INIST
- 3629026
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
10.1029/95JA00522 
https://dx.doi.org/10.1029/95JA00522
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