Possible wave amplitudes in shocks in the solar corona : predictions for solar probe
- Author
- MOSES, S. L1 ; CORONITI, F. V; GREENSTADT, E. W; TSURUTANI, B. T
[1] TRW, space technology group, Redondo Beach CA 90278, United States - Source
JGR. Journal of geophysical research. Part A, Space physics. 1991, Vol 96, Num 12, pp 21397-21401 ; ref : 1/2 p
- CODEN
- JJGPD4
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- American Geophysical Union, Washington, DC
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Accélération particule Chauffage plasma Couronne solaire Observation par satellite Onde Alfvén Onde choc MHD Onde choc magnétosphérique Satellite ISEE 3
- Keyword (en)
- Particle acceleration Plasma heating Solar corona Satellite observation Alfven wave MHD shock wave Magnetospheric shock wave
- Keyword (es)
- Aceleración partícula Calentamiento plasma Corona solar Observación por satélite Onda Alfven Onda choque MHD Onda choque magnetoesférica
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B60 Solar physics / 001E03B60P Corona. Coronal loops, streamers, and holes
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 5027290
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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DOI
10.1029/91JA02268 
https://dx.doi.org/10.1029/91JA02268
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