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On the formation of the high-altitude stagnant cusp : Cluster observations

Author
BOGDANOVA, Y. V1 ; MARCHAUDON, A1 ; OWEN, C. J1 ; DUNLOP, M. W2 ; FREY, H. U3 ; WILD, J. A4 ; FAZAKERLEY, A. N1 ; KLECKER, B5 ; DAVIES, J. A2 ; MILAN, S. E4
[1] Milliard Space Science Laboratory, University College London, Dorking, United Kingdom
[2] Space Science and Technology Department, Rutherford Appleton Laboratory, Didcot, United Kingdom
[3] Space Science Laboratory, University of California, Berkeley, California, United States
[4] Department of Physics and Astronomy, University of Leicester, Leicester, United Kingdom
[5] Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany
Source

Geophysical research letters. 2005, Vol 32, Num 12, pp L12101.1-L12101.5 ; ref : 16 ref

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
English
Keyword (fr)
Convection Gaine magnétosphérique Haute altitude Haute latitude Hémisphère Nord Hémisphère Sud Injection Ligne force Modèle Plasma Marches Europe Europe Sud Italie
Keyword (en)
convection Magnetosheath High altitude High latitude Northern Hemisphere Southern Hemisphere injection Field line models Plasma Marches Italy Europe Southern Europe Italy
Keyword (es)
Convección Vaina magnetosférica Gran altura Alta latitud Hemisferio norte Hemisferio sur Inyección Línea fuerza Modelo Plasma Marcas Europa Europa Sur Italia
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E01 Earth sciences

Discipline
Earth sciences
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16988987

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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