Bow shock 'splitting' in bi-ion flows
- Autor
- SAUER, K1 ; DUBININ, E1 2 ; BAUMGÄRTEL, K1 ; BOGDANOV, A3
[1] Max-Planck-Institut für estratterestrische Physik, Aussenstelle Berlin, Germany
[2] Space Research Institute, Russian Academy of Sciences, Moscow, Russian Federation
[3] Max-Planck-Instiut für extraterrestrische Physik, Garching, Germany - Fuente
Geophysical research letters. 1996, Vol 23, Num 24, pp 3643-3646 ; ref : 20 ref
- CODEN
- GPRLAJ
- ISSN
- 0094-8276
- Campo Científico
- Astronomy earth cosmic environment; Geophysics; Climatology, meteorology; Oceanography
- Editor
- American Geophysical Union, Washington, DC
- País de la publicación
- United States
- Tipo de documento
- Article
- Idioma
- Russian
- Palabra clave (fr)
- Comète Discontinuité Ecoulement plasma Ion lourd Modèle 2 dimensions Onde choc magnétosphérique Planète Mars Plasma sans collision Proton cosmique Simulation numérique Vent solaire
- Palabra clave (in)
- Comets Discontinuity Plasma flow Heavy ions Two dimensional model Bow shock Mars planet Collisionless plasma Cosmic protons Numerical simulation Solar wind
- Palabra clave (es)
- Discontinuidad Modelo 2 dimensiones Simulación numérica
- Clasificación
- 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
- 2501539
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
10.1029/96GL03425 
https://dx.doi.org/10.1029/96GL03425
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