Shell models of RMHD turbulence and the heating of solar coronal loops

Astrophysical Journal

Volumn 662, Issue 1 I, 2007, Pages 701-714

  Buchlin, E ^a,b   Velli, M ^a,c  

^a UNIVERSITY OF FLORENCE   (Italy)

^b IMPERIAL COLLEGE LONDON   (United Kingdom)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

MHD; Sun: corona; Sun: flares; Turbulence

Indexed keywords

EID: 34250860715     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/512765     Document Type: Article

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