Magnetic tornadoes as energy channels into the solar corona

被引：0

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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D O I：

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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.

引用

页码：505 / 508

页数：3

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