Fast damping of acoustic waves in solar coronal loops as a result of their radiation

Fast damping of acoustic waves in solar coronal loops as a result of their radiation

The problem of the observed fast damping of longitudinal waves in solar coronal magnetic loops is studied. According to some data, the radiation effect, which plays a key role in the cooling of coronal loops that are observed in the extreme UV wavelength range, is used to explain this phenomenon. Th...

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Veröffentlicht in:Geomagnetism and Aeronomy 2013-12, Vol.53 (8), p.1013-1015
Hauptverfasser: Bembitov, D. B., Veselovsky, I. S., Mikhalyaev, B. B.
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Sprache:eng
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Corona
Damping
Earth and Environmental Science
Earth Sciences
Geophysics/Geodesy
Magnetic fields
Radiation
Solar energy
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container_issue 8
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container_title Geomagnetism and Aeronomy
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creator Bembitov, D. B.
Veselovsky, I. S.
Mikhalyaev, B. B.
description The problem of the observed fast damping of longitudinal waves in solar coronal magnetic loops is studied. According to some data, the radiation effect, which plays a key role in the cooling of coronal loops that are observed in the extreme UV wavelength range, is used to explain this phenomenon. The dispersion relation for slow magnetosonic modes of a cylindrical magnetic tube has been obtained with regard to the radiation effect. It has been indicated that the radiation actually results in the fast damping of the slow magnetosonic modes of coronal magnetic loops.
doi_str_mv 10.1134/S0016793213080033
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source Springer Nature - Complete Springer Journals
subjects Corona
Damping
Earth and Environmental Science
Earth Sciences
Geophysics/Geodesy
Magnetic fields
Radiation
Solar energy
title Fast damping of acoustic waves in solar coronal loops as a result of their radiation
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