Forward modeling of hot loop oscillations observed by SUMER and SXT
- Author
- TAROYAN, Y1 ; ERDELYI, R1 ; WANG, T. J2 ; BRADSHAW, S. J3
[1] Solar Physics and Space Plasma Research Centre, Department of Applied Mathematics, University of Sheffield, Sheffield, S3 7RH, United Kingdom
[2] Department of Physics, Montana State University, Bozeman, MT 59717-3840, United States
[3] Space and Atmospheric Physics, Blackett Laboratory, Imperial College London, Prince Consort Road, London SW7 2BZ, United Kingdom - Source
The Astrophysical journal. 2007, Vol 659, Num 2 ; L173-L176 ; 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
- hydrodynamics line: profiles-Sun: atmosphere-Sun: oscillations color figures
- Keyword (fr)
- Couleur Modélisation Profil raie Soleil
- Keyword (en)
- Color Modelling Line shape Sun
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18716687
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
10.1086/517521 
https://dx.doi.org/10.1086/517521
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