Linear theory of oblique Alfve'n and rapid magnetosound waves in the magnetosphere.

Details Linear theory of oblique Alfve'n and rapid magnetosound waves in the magnetosphere. Linear theory of oblique Alfve'n and rapid magnetosound waves in the magnetosphere.

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990cosre..28..226c&link_type=abstract

Cosmic Res., Vol. 28, No. 2, p. 226 - 234

Computer Science

Sound

Earth Magnetosphere: Alfven Waves

Scientific paper

The authors consider the linear interaction of oblique Alfve'n and rapid magnetosound waves with the particles of the magnetospheric plasma. They obtain the refractive index for a sufficiently broad frequency region and propagation angles. They calculate the Cherenkov decrements of wave damping on cold and hot plasma components and analyze the instability on the ion-cyclotron resonances. They determine the instability region for both types of waves as a function of the parameters of the hot plasma of the magnetosphere ring current, frequency, and propagation angle.

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