Interoccurrence times in the Bak-Tang-Wiesenfeld sandpile model : A comparison with the observed statistics of solar flares
- Author
- PACZUSKI, Maya1 ; BOETTCHER, Stefan2 ; BAIESI, Marco3
[1] Perimeter Institute for Theoretical Physics, Waterloo, N2L 2Y5, Canada
[2] Department of Physics, Emory University, Atlanta, Georgia 30322, United States
[3] Instituut voor Theoretische Fysica, K. U. Leuven, 3001, Belgium - Source
Physical review letters. 2005, Vol 95, Num 18, pp 181102.1-181102.4 ; ref : 49 ref
- CODEN
- PRLTAO
- ISSN
- 0031-9007
- Scientific domain
- Optics; Atomic molecular physics; Condensed state physics; Physics; Plasma physics
- Publisher
- American Physical Society, Ridge, NY
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Eruption chromosphérique Modèle tas sable Statistique 9660R
- Keyword (en)
- Solar flare Sandpile models Statistics
- Keyword (es)
- Erupción cromosférica
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B60 Solar physics / 001E03B60R Flares, bursts, and related phenomena
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17291266
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
10.1103/PhysRevLett.95.181102 
https://dx.doi.org/10.1103/PhysRevLett.95.181102
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