New evidence for the role of emerging flux in a solar Filament's slow rise preceding its cme-producing fast eruption
- Author
- STERLING, Alphonse C1 ; HARRA, Louise K2 ; MOORE, Ronald L1
[1] NASA Marshall Space Flight Center, Space Science Office, VP62, Huntsville, AL 35805, United States
[2] Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom - Source
The Astrophysical journal. 2007, Vol 669, Num 2, pp 1359-1371, 13 p ; 1 ; ref : 1/2 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- Sun: UV radiation Sun: X-rays, gamma rays Sun: coronal mass ejections (CMEs) Sun: filaments Sun: flares
- Keyword (fr)
- Ejection masse coronale Filament Flux solaire Rayonnement UV Rayonnement gamma Soleil
- Keyword (en)
- Coronal mass ejection Filaments Solar flux Ultraviolet radiation Gamma radiation Sun
- Keyword (es)
- Eyección masa coronal
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19240200
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
10.1086/520829 
https://dx.doi.org/10.1086/520829
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