Coronal heating by prominence turbulence

Details Coronal heating by prominence turbulence Coronal heating by prominence turbulence

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...66...29v&link_type=abstract

Solar Physics, vol. 66, May 1980, p. 29-37. Research supported by the Nederlandse Organisatie voor Zuiver-Wettenschappelijk Onde

Physics

1

Atmospheric Turbulence, Magnetohydrodynamic Waves, Plasma Heating, Solar Corona, Solar Prominences, Wave Generation, Chromosphere, Conductive Heat Transfer

Scientific paper

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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