Modelling the global solar corona II: Coronal evolution and filament chirality comparison

Solar Physics

Volumn 247, Issue 1, 2008, Pages 103-121

  Yeates, A R ^a   MacKay, D H ^a   Van Ballegooijen, A A ^b  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Helicity: magnetic; Magnetic fields: corona; Prominences: magnetic field

Indexed keywords

EID: 38349088044     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/s11207-007-9097-0     Document Type: Article

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