Modeling the radiative signatures of turbulent heating in coronal loops
- Author
- PARENT, S1 ; BUCHLIN, E2 ; CARGILL, P. J3 ; GALTIER, S1 4 ; VIAL, J.-C1 4
[1] Institut d'Astrophysique Spatiale, Batiment 121, 91405 Orsay, France
[2] Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, Largo E. Fermi 2, 50125 Florence, Italy
[3] Space and Atmospheric Physics, Blackett Laboratory, Imperial College, London SW7 2BZ, United Kingdom
[4] Université Paris-Sud 11 and CNRS (UMR 8617), France - Source
The Astrophysical journal. 2006, Vol 651, Num 2, pp 1219-1228, 10 p ; 1 ; ref : 38 ref
- 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
- MHD Sun: UV radiation Sun: corona Sun: flares methods: statistical techniques: spectroscopic turbulence
- Keyword (fr)
- Boucle coronale Chauffage turbulent Modélisation Méthode statistique Rayonnement UV Soleil Turbulence
- Keyword (en)
- Coronal loop Turbulent heating Modelling Statistical method Ultraviolet radiation Sun Turbulence
- Keyword (es)
- Bucle coronal Método estadístico
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18353943
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
10.1086/507594 
https://dx.doi.org/10.1086/507594
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