Coronal heating by prominence turbulence |
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| Authors: | W Van Tend |
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| Institution: | (1) The Astronomical Institute at Utrecht, Sterrewacht, Zonnenburg 2, 3512 Utrecht, NL, The Netherlands |
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| Abstract: | The generation of magnetohydrodynamic waves in the corona by the observed random motions in prominences is considered. The associated energy input into the corona may be a significant source of heating for the coronal loops overlying prominences, especially during the onset of flares. Some relevant observations are discussed. |
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