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Reconnection onset in the magnetotail: Particle simulations with open boundary conditions

Author
DIVIN, A. V1 ; SITNOV, M. I2 ; SWISDAK, M2 3 ; DRAKE, J. F2
[1] Institute of Physics, St. Petersburg University, St. Petersburg, Russian Federation
[2] Institute for Research in Electronics and Applied Physics, University of Maryland, College Park, Maryland, United States
[3] Naval Research Laboratory, Washington, D. C, United States
Source

Geophysical research letters. 2007, Vol 34, Num 9 ; L09109.1-L09109.5 ; ref : 1/4 p

CODEN
GPRLAJ
ISSN
0094-8276
Scientific domain
Astronomy earth cosmic environment; Geophysics; Climatology, meteorology; Oceanography
Publisher
American Geophysical Union, Washington, DC
Publication country
United States
Document type
Article
Language
Russian
Keyword (fr)
Code particule Condition aux limites Couronne solaire Gemme Géométrie Instabilité déchirure Ion Magnétosphère planétaire Modélisation Particule Physique plasma Plasma sans collision Queue magnétosphérique Reconnexion magnétique Simulation Sous orage magnétosphérique
Keyword (en)
Particle code boundary conditions Solar corona gems geometry Tearing instability ions Planetary magnetospheres Modeling particles Plasma physics Collisionless plasma Magnetospheric tail Magnetic reconnection simulation Magnetospheric substorm
Keyword (es)
Código partícula Condiciones límites Corona solar Gema Geometría Inestabilidad desgarrón Ión Modelización Física plasma Plasma sin colisión Cola magnetosférica Simulación Subtormenta magnetoesférica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18822706

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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