Three-dimensional MHD wave propagation and conversion to Alfvén waves near the solar surface. I. Direct numerical solution

Solar Physics

Volumn 251, Issue 1-2, 2008, Pages 251-265

  Cally, P S ^a,b   Goossens, M ^b  

^a MONASH UNIVERSITY   (Australia)

^b CENTRE FOR PLASMA ASTROPHYSICS   (Belgium)

Author keywords

Helioseismology: theory; Waves: magnetohydrodynamic

Indexed keywords

EID: 50249162102     PISSN: 00380938     EISSN: 1573093X     Source Type: Journal    
DOI: 10.1007/s11207-007-9086-3     Document Type: Article

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