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Reasons why some solar wind changes do not trigger substorms

Author
LEE, D.-Y1 ; LYONS, L. R2 ; WEYGAND, James M3 ; WANG, C.-P2
[1] Department of Astronomy and Space Science, College of Natural Sciences and Institute for Basic Science Research, Chungbuk National University, Chungbuk, Korea, Republic of
[2] Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, California, United States
[3] Institute of Geophysics and Planetary Physics, Department of Earth and Space Sciences, University of California, Los Angeles, California, United States
Source

Journal of geophysical research. 2007, Vol 112, Num A6 ; A06240.1-A06240.17 ; 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)
Champ magnétique interplanétaire Convection Couche plasma Direction Déclenchement Phase croissance orage Pression dynamique Résistance mécanique Vent solaire
Keyword (en)
Interplanetary magnetic field convection Plasma layer direction Triggering Growth phase magnetic storm Dynamic pressure strength solar wind
Keyword (es)
Campo magnético interplanetario Convección Capa plasma Dirección Inducción Fase crecimiento tormenta Presión dinámica Resistencia mecánica Viento solar
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18963774

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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