Magnetohydrodynamic phenomena in the solar atmosphere.

Details Magnetohydrodynamic phenomena in the solar atmosphere. Magnetohydrodynamic phenomena in the solar atmosphere.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ppmto..13...87f&link_type=abstract

Publ. Purple Mt. Obs., Vol. 13, No. 2, p. 87 - 97

Physics

Solar Atmosphere: Magnetohydrodynamics

Scientific paper

Solar atmosphere is a rotating plasma shell filled by magnetic field. The coupling between the magnetic and the movement of plasma makes a variety of magnetohydrodynamic phenomena in the solar atmosphere. After a brief introduction on the basic theoretical regime of solar MHD, the authors describe mainly the magnetohydrodynamic aspects of solar flares, solar prominences (filaments) and flux tubes with different scales.

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