Coronal loops heated by magnetohydrodynamic turbulence. I. A model of isobaric quiet-sun loops with constant cross sections

Astrophysical Journal

Volumn 581, Issue 1 I, 2002, Pages 726-735

  Chae, Jongchul ^a,b   Poland, Arthur I ^c   Aschwanden, Markus J ^d  

^a Chungnam National University   (South Korea)

^b NEW JERSEY INSTITUTE OF TECHNOLOGY   (United States)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d LOCKHEED MARTIN   (United States)

Author keywords

MHD; Sun: corona; Sun: magnetic fields; Sun: transition region; Turbulence

Indexed keywords

EID: 0042133349     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/344103     Document Type: Article

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