Solar magnetoatmospheric waves - A simplified mathematical treatment

Details Solar magnetoatmospheric waves - A simplified mathematical treatment Solar magnetoatmospheric waves - A simplified mathematical treatment

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....60..171a&link_type=abstract

Astronomy and Astrophysics, vol. 60, no. 2, Sept. 1977, p. 171-179.

Astronomy and Astrophysics

Astrophysics

8

Magnetoacoustic Waves, Magnetohydrodynamic Waves, Solar Atmosphere, Solar Magnetic Field, Stellar Models, Group Velocity, Magnetic Effects, Shock Waves, Wave Equations

Scientific paper

The inhomogeneous wave equation for a special class of magnetoatmospheric waves is formally solved, and the principle of stationary phase used to provide information on the group-velocity properties of such waves. General results are presented concerning the associated mechanical energy flux. The basic problem considered is relevant to waves initiated by sudden events in the solar atmosphere.

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