Singularities of the local MHD-resonances in solar chromosphere plasma

Details Singularities of the local MHD-resonances in solar chromosphere plasma Singularities of the local MHD-resonances in solar chromosphere plasma

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work..111l&link_type=abstract

In ESA, Proceedings of an Internatinal School and Workshop on Plasma Astrophysics, Volume 1 p 111-114 (SEE N89-24910 18-75)

Physics

Plasma Physics

Chromosphere, Plasma Heating, Plasma Resonance, Polar Cusps, Solar Atmosphere, Solar Oscillations, Convective Flow, Magnetohydrodynamic Flow, Plasma Oscillations, Plasma Physics, Solar Wind

Scientific paper

The dissipation of the energy of the forced oscillations stipulated by convective motions at the Sun, in the local cusp-resonance regions in the high Beta chromosphere plasma is considered. If the Alfven velocity has the extremum in the resonance point the width of the resonance region and the power absorption increase. Conditions when the nonlinear effects become essential and may lead to the forming of the nonlinear (discontinuous) flows in the cusp-layer are obtained.

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