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Storm-substorm relationship: Contribution of the tail current to Dst

Author
OHTANI, S1 ; NOSE, M1 ; ROSTOKER, G2 ; SINGER, H3 ; LUI, A. T. Y1 ; NAKAMURA, M4
[1] The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, United States
[2] Solar-Terrestrial Environmental Laboratory, Nagoya University, Toyokawa, Japan
[3] National Oceanic and Atmospheric Administration, Boulder, Colorado, United States
[4] Department of Earth and Planetary Physics, University of Tokyo, Tokyo, Japan
Source

Journal of geophysical research. 2001, Vol 106, Num A10, pp 21199-21209 ; ref : 28 ref

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)
Analyse statistique Champ magnétique interplanétaire Champ magnétique Courant annulaire Courant électrique Observation par satellite Orage magnétique Phase rétablissement orage Queue magnétosphérique Satellite GOES Satellite Geotail Source courant Sous orage magnétosphérique Variation Dst
Keyword (en)
Statistical analysis Interplanetary magnetic field Magnetic field Ring current Electric current Satellite observation Magnetic storm Recovery phase magnetic storm Magnetospheric tail GOES satellites Geotail satellite Current source Magnetospheric substorm Dst variation
Keyword (es)
Análisis estadístico Campo magnético interplanetario Campo magnético Corriente anular Corriente eléctrica Observación por satélite Tormenta magnética Fase restablecimiento tormenta Cola magnetosférica Satélite Geotail Fuente corriente Subtormenta magnetoesférica Variación Dst
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E02 External geophysics / 001E02J Physics of the magnetosphere / 001E02J05 Magnetic storms, substorms

Discipline
External geophysics
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
14097839

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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