An assessment of magnetic conditions for strong coronal heating in solar active regions by comparing observed loops with computed potential field lines

Astrophysical Journal

Volumn 528, Issue 2 PART 1, 2000, Pages 1004-1014

  Falconer, D A ^a   Gary, G A ^b   Moore, R L ^b   Porter, J G ^b  

^a UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^b NASA MARSHALL SPACE FLIGHT CENTER   (United States)

Author keywords

Sun: Corona; Sun: Magnetic fields; Sun: X rays, gamma rays

Indexed keywords

EID: 0034627515     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/308188     Document Type: Article

References (11)

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