Trapped waves in open stellar atmospheres.

Details Trapped waves in open stellar atmospheres. Trapped waves in open stellar atmospheres.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pobeo..54...59p&link_type=abstract

Publications of the Astronical Observatory of Belgrade, No. 54, p. 59 - 62

Astronomy and Astrophysics

Astronomy

Stellar Atmospheres: Models, Stellar Atmospheres: Magnetohydrodynamics

Scientific paper

Linear MHD waves whose energy remains localized in an unbounded stellar atmosphere are considered analytically and numerically. The atmosphere is modelled by a stratified fully ionized plasma with both the gravity force and the gradient of the unperturbed fluid quantities aligned along the vertical z-axis. The temperature is taken to have a linear profile while the magnetic field is assumed horizontal and homogeneous. The atmosphere is semi-infinite with a solid boundary at its bottom (the stellar photosphere). In such a system, the authors are looking for solutions localized in space and that could be treated as eigenmodes.

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