Alfvénic waves with sufficient energy to power the quiet solar corona and fast solar wind
Scott W. McIntoshHigh Altitude Observatory, National Center for Atmospheric Research, PO Box 3000, Boulder, Colorado 80307, USA. [email protected]Bart De PontieuLockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Palo Alto, 94304, California, USAM. CarlssonInstitute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, NorwayV. H. HansteenInstitute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, 0315 Oslo, NorwayP. BoernerLockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Palo Alto, 94304, California, USAM. GoossensDepartment of Mathematics, Centre for Plasma Astrophysics, Katholieke Universiteit Leuven, Celestijnenlaan 200B, B-3001 Heverlee, Belgium
2011en
ABI
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