Magnetoacoustic heating of the solar chromosphere

Details Magnetoacoustic heating of the solar chromosphere Magnetoacoustic heating of the solar chromosphere

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...381l..31d&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 381, Nov. 1, 1991, p. L31-L33.

Computer Science

Sound

3

Chromosphere, Magnetoacoustics, Plasma Heating, Solar Atmosphere, Convection, Emission Spectra, Sound Waves, Stellar Magnetic Fields, Stellar Models

Scientific paper

Long-period acoustic waves generated in the solar convection zone can propagate radially outward through the overlying atmosphere and get resonantly absorbed in the magnetic arches of the low-lying chromospheric canopy. The resulting Poynting and acoustic flux that enters the magnetic canopy in the network regions is demonstrated to be adequate to account for the observed chromospheric emission.

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