Computer Science – Numerical Analysis
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phfl...31..547h&link_type=abstract
Physics of Fluids (ISSN 0031-9171), vol. 31, March 1988, p. 547-561.
Computer Science
Numerical Analysis
4
Magnetoacoustic Waves, Magnetohydrodynamic Waves, Plasma Conductivity, Thermal Conductivity, Astrophysics, Magnetic Fields, Numerical Analysis, Perturbation Theory, Solar Physics
Scientific paper
The linear spectrum of one-dimensional magnetostatic and thermally conducting plasmas is analyzed. The model and mathematical expressions for the eigenvalue problem of linear motions of a one-dimensional plasma in a gravitational field are presented. The effects of thermal conduction on the linear spectrum, the ideal slow continuous spectrum, and the isothermal slow continuous spectrum are investigated. Particular attention is given to changes in the slow and fast magnetoacoustic modes and the thermal modes of the isothermal slow continuous spectrum. It is observed that thermal conduction affects various portions of the linear spectrum of ideal MHD differently; the ideal Alfven continuous spectrum is not influenced by thermal conduction; and the isothermal slow continuous spectrum replaces the ideal slow continuous spectrum.
Goossens Marcel
Hermans D.
Kerner Wolfgang
Lerbinger K.
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