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Electron flux spectral imaging of solar flares through regularized analysis of hard x-ray source visibilities

Author
PIANA, Michele1 ; MASSONE, Anna Maria2 ; HURFORD, G. J3 ; PRATO, Marco4 ; GORDON EMSLIE, A5 ; KONTAR, Eduard P6 ; SCHWARTZ, Richard A7
[1] Dipartimento di Informatica, Università di Verona, Ca' Vignal 2, Strada le Grazie 15, 37134 Verona, Italy
[2] CNR-INFM LAMIA, via Dodecaneso 33, 16145 Genova, Italy
[3] Space Sciences Laboratory, University of California, Berkeley, 8 Gauss Way, Berkeley, CA 94720-7450, United States
[4] Dipartimento di Matematica, Universita di Modena e Reggio Emilia, via Campi 213/b, 41100 Modena, Italy
[5] Department of Physics, Oklahoma State University, Stillwater, OK 74078, United States
[6] Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, Scotland, United Kingdom
[7] CUA (Catholic University) and LSSP at NASA Goddard Space Flight Center, code 671.1, Greenbelt, MD 20771, United States
Source

The Astrophysical journal. 2007, Vol 665, Num 1, pp 846-855, 10 p ; 1 ; 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: X-rays, gamma rays Sun: flares methods: data analysis techniques: image processing techniques: spectroscopic
Keyword (fr)
Analyse donnée Eruption solaire Flux électrons Rayon X dur Rayonnement gamma Soleil Traitement image Visibilité
Keyword (en)
Data analysis Solar flares Electron flux Hard x radiation Gamma radiation Sun Image processing Visibility
Keyword (es)
Flujo electrones
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18990663

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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