Alfven surface waves along coronal streamers

Details Alfven surface waves along coronal streamers Alfven surface waves along coronal streamers

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.109..357n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 109, no. 2, Feb. 1985, p. 357-364.

Astronomy and Astrophysics

Astrophysics

7

Magnetohydrodynamic Waves, Solar Corona, Surface Waves, Magnetohydrodynamic Stability, Wave Dispersion

Scientific paper

The dispersive characteristics of Alfven surface waves for a moving plasma surrounded by a stationary plasma are discussed. The dispersion and stability curves for the symmetric and asymmetric modes are presented. The results indicate that the interface parameters eta and beta-squared, where eta is the density ratio and beta-squared is the magnetic field ratio, significantly affect the phase velocities of the modes. The stability properties of the waves are found to be dependent on the combined effect of the interface parameters.

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