Statistics – Computation
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acaps...6..231w&link_type=abstract
(Acta Astrophysica Sinica, vol. 6, 1986, p. 231-239) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, Dec. 1986, p.
Statistics
Computation
Gravity Waves, Magnetoacoustic Waves, Solar Atmosphere, Solar Magnetic Field, Wave Propagation, Atmospheric Temperature, Computational Astrophysics, Polarization Characteristics, Surface Waves
Scientific paper
An analysis of magnetoacoustic-gravity waves in the case of an isothermal atmosphere permeated by a uniform magnetic field is presented. The general solution is expressed in terms of generalized hypergeometric functions. It can be used in numerical simulation of oscillations in a magnetic atmosphere. It is shown that the elliptically polarized magnetoacoustic-gravity wave consist of a pair of surface waves and a pair of body waves above the cut-off frequency. The body waves along the magnetic field are similar to acoustic waves in an atmosphere, and their cut-off frequency is unaffected by magnetic field. The transverse oscillation decreases with height. For the usual boundary condition, the longitudinal oscillation decreases with height; however, in some cases, it may contain terms that increase with height. The solution is singular on a family of ellipses in the frequency - horizontal wave number plane. Near these ellipses, the wave components grow indefinitely.
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