NON-GAUSSIAN LINE PROFILES IN A LARGE SOLAR FLARE OBSERVED ON 2006 DECEMBER 13
- Author
- IMADA, S1 ; HARA, H1 ; WATANABE, T1 ; ASAI, A2 ; MINOSHIMA, T3 ; HARRA, L. K4 ; MARISKA, J. T5
[1] National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka-shi, Tokyo 181-8588, Japan
[2] Nobeyama Solar Radio Observatory, Minamisaku, Nagano 384-1305, Japan
[3] Department of Earth and Planetary Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
[4] UCL-Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom
[5] Space Science Division, Naval Research Laboratory, Washington, DC 20375, United States - Source
The Astrophysical journal. 2008, Vol 679, Num 2 ; L155-L159 ; 2 ; ref : 1/4 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: corona-Sun: flares
- Keyword (fr)
- Eruption solaire Loi normale Profil raie Soleil
- Keyword (en)
- Solar flares Normal distribution Line shape Sun
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20389509
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
10.1086/589444 
https://dx.doi.org/10.1086/589444
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