Magnetic tornadoes as energy channels into the solar corona

被引：0
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作者：
Sven Wedemeyer-Böhm
Eamon Scullion
Oskar Steiner
Luc Rouppe van der Voort
Jaime de la Cruz Rodriguez
Viktor Fedun
Robert Erdélyi
机构：
[1] Institute of Theoretical Astrophysics,Department of Physics and Astronomy
[2] University of Oslo,undefined
[3] PO Box 1029 Blindern,undefined
[4] N-0315 Oslo,undefined
[5] Norway ,undefined
[6] Center of Mathematics for Applications,undefined
[7] University of Oslo,undefined
[8] PO Box 1053 Blindern,undefined
[9] N-0316 Oslo,undefined
[10] Norway ,undefined
[11] Kiepenheuer Institute for Solar Physics,undefined
[12] Schöneckstrasse 6–7,undefined
[13] D-79104 Freiburg,undefined
[14] Germany ,undefined
[15] Uppsala University,undefined
[16] Box 516,undefined
[17] SE-75120 Uppsala,undefined
[18] Sweden,undefined
[19] Solar Physics and Space Plasma Research Centre,undefined
[20] School of Mathematics and Statistics,undefined
[21] University of Sheffield,undefined
[22] Hicks Building,undefined
[23] Hounsfield Road,undefined
[24] Sheffield S3 7RH,undefined
[25] UK ,undefined
来源：
Nature | 2012年 / 486卷
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摘要：
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.
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页码：505 / 508
页数：3
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