The generation of MHD waves by forced turbulence in a weakly magnetized fluid

Details The generation of MHD waves by forced turbulence in a weakly magnetized fluid The generation of MHD waves by forced turbulence in a weakly magnetized fluid

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...219l..27r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 219, no. 1-2, July 1989, p. L27-L29.

Astronomy and Astrophysics

Astrophysics

4

Magnetohydrodynamic Waves, Solar Corona, Turbulence Effects, Wave Generation, Buoyancy, Emission Spectra, Wave Propagation

Scientific paper

The effect of the fluctuating buoyancy force on wave generation in a weakly magnetized plasma is considered. As expected, the efficiency of MHD wave generation is enhanced by including this force. However, it remains true that the observed variation of coronal emission at fixed spectral type cannot be accounted for by a wave generation process of the type discussed here.

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