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Differences in the O7+/O6+ ratio of magnetic cloud and non-cloud Coronal Mass ejections

Author
HENKE, T1 ; WOCH, J1 ; MALL, U1 ; LIVI, S1 ; WILKEN, B1 ; SCHWENN, R1 ; GLOECKLER, G2 ; VON STEIGER, R3 ; FORSYTH, R. J4 ; BALOGH, A4
[1] Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany
[2] University of Maryland, College Park, Maryland, United States
[3] International Space Science Institute, Bern, Switzerland
[4] Blackett Laboratory, Imperial College, London, United Kingdom
Source

Geophysical research letters. 1998, Vol 25, Num 18, pp 3465-3468 ; ref : 18 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)
Ejection masse coronale Etat charge Nuage magnétique Oxygène ion Sonde spatiale Ulysse Structure magnétique Vent solaire
Keyword (en)
Coronal mass ejection Charge states Magnetic cloud Oxygen ions Ulysses space probes Magnetic structure Solar wind
Keyword (es)
Eyección masa coronal Nube magnetica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B50 Interplanetary space / 001E03B50C Solar wind plasma

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
1610455

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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