Model prediction for an observed filament

Astrophysical Journal

Volumn 543, Issue 1 PART 1, 2000, Pages 447-456

  Aulanier, G ^a   Srivastava, N ^b   Martin, S F ^c  

^a NAVAL RESEARCH LABORATORY   (United States)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^c Helio Research   (United States)

Author keywords

MHD; Sun: filaments; Sun: magnetic fields; Sun: prominences

Indexed keywords

EID: 0034311421     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/317095     Document Type: Article

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