Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.189..223b&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 189, no. 2, March 1992, p. 223-235. Research supported by Swedish Agency f
Astronomy and Astrophysics
Astrophysics
Compressible Flow, Magnetohydrodynamic Flow, Plasma Composition, Reacting Flow, Solar Flares, Thermal Radiation, Boussinesq Approximation, Channel Flow, Hydrogen, Integral Equations, Optical Thickness
Scientific paper
The paper studies the compressible flow of a hot two-component plasma in the presence of gravitation and chemical reaction in a vertical channel. For the optically thick gas appoximation, closed form analytical solutions are possible. Asymptotic solutions are also obtained for the general differential approximation when the temperatures of the two bounding walls are the same. In the general case the problem is reduced to the solution of standard nonlinear integral equations which can be tackled by iterative procedure. The results are discussed quantitatively. The problem may be applicable to the understanding of explosive hydrogen-burning model of solar flares.
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