On heating the sun's corona by magnetic explosions: Feasibility in active regions and prospects for quiet regions and coronal holes

Astrophysical Journal

Volumn 526, Issue 1 PART 1, 1999, Pages 505-522

  Moore, R L ^a   Falconer, D A ^b   Porter, J G ^a   Suess, S T ^a  

^a NASA MARSHALL SPACE FLIGHT CENTER   (United States)

^b UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

Author keywords

MHD; Sun: corona; Sun: magnetic fields; Sun: X rays, gamma rays

Indexed keywords

EID: 0033589631     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/307969     Document Type: Article

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