Astronomy and Astrophysics
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.
Original Publication Citation
Adam, J. A. (1977). Solar magnetoatmospheric waves-a simplified mathematical treatment. Astronomy and Astrophysics, 60(2), 171-179.
Adam, John A., "Solar Magnetoatmospheric Waves-a Simplified Mathematical Treatment" (1977). Mathematics & Statistics Faculty Publications. 181.