Magnetic tornadoes as energy channels into the solar corona
Sven Wedemeyer-Böhm (),
Eamon Scullion,
Oskar Steiner,
Luc Rouppe van der Voort,
Jaime de la Cruz Rodriguez,
Viktor Fedun and
Robert Erdélyi
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Sven Wedemeyer-Böhm: Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, N-0315 Oslo, Norway
Eamon Scullion: Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, N-0315 Oslo, Norway
Oskar Steiner: Kiepenheuer Institute for Solar Physics, Schöneckstrasse 6–7, D-79104 Freiburg, Germany
Luc Rouppe van der Voort: Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029 Blindern, N-0315 Oslo, Norway
Jaime de la Cruz Rodriguez: Uppsala University, Box 516, SE-75120 Uppsala, Sweden
Viktor Fedun: Solar Physics and Space Plasma Research Centre, School of Mathematics and Statistics, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK
Robert Erdélyi: Solar Physics and Space Plasma Research Centre, School of Mathematics and Statistics, University of Sheffield, Hicks Building, Hounsfield Road, Sheffield S3 7RH, UK
Nature, 2012, vol. 486, issue 7404, 505-508
Abstract:
Rotating magnetic structures in the Sun can channel energy outwards from the convection zone and may explain how the energy required to heat the outer layers of the Sun reaches its upper atmosphere.
Date: 2012
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DOI: 10.1038/nature11202
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