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Plasmoid formation for multiple onset substorms : observations of the Japanese Lunar Mission Kaguya

Author
NAGAI, T1 ; TSUNAKAWA, H1 ; SAITO, Y4 ; AMM, O5 ; SHIBUYA, H2 ; TAKAHASHI, F1 ; SHIMIZU, H3 ; MATSUSHIMA, M1 ; NISHINO, M. N4 ; YOKOTA, Y4 ; ASAMURA, K4 ; TANAKA, T4
[1] Tokyo Institute of Technology, Tokyo, Japan
[2] Kumamoto University, Kumamoto, Japan
[3] University of Tokyo, Tokyo, Japan
[4] Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan
[5] Finnish Meteorological Institute, Helsinki, Finland
Source

Annales geophysicae (1988). 2009, Vol 27, Num 1, pp 59-64, 6 p ; ref : 3/4 p

ISSN
0992-7689
Scientific domain
Astronomy earth cosmic environment; Geophysics
Publisher
Copernicus, Göttingen
Publication country
Germany
Document type
Article
Language
English
Author keyword
Magnetospheric physics (Magnetotail; Storms and substorms) Space plasma physics (Magnetic reconnection)
Keyword (fr)
Champ magnétique Ligne force Physique plasma Plasma Plasmoïde Queue magnétosphérique Reconnexion magnétique Région compression itinérante Tempête
Keyword (en)
magnetic field Field line Plasma physics Plasma Plasmoid Magnetospheric tail Magnetic reconnection Traveling compression region storms
Keyword (es)
Campo magnético Línea fuerza Física plasma Plasma Plasmoide Cola magnetosférica Región compresión itinerante Tempestad
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E02 External geophysics / 001E02I Physics of the ionosphere

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E02 External geophysics / 001E02J Physics of the magnetosphere

Discipline
External geophysics
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
21271431

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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