Heating of the Solar Chromosphere and Corona by Alfvén Wave Turbulence
A three-dimensional magnetohydrodynamic (MHD) model for the propagation and dissipation of Alfven waves in a coronal loop is developed. The model includes the lower atmospheres at the two ends of the loop. The waves originate on small spatial scales (less than 100 km) inside the kilogauss flux eleme...
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Published in | The Astrophysical journal Vol. 736; no. 1; pp. 3 - jQuery1323905833864='48' |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
United States
IOP Publishing
20.07.2011
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Subjects | |
Online Access | Get full text |
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