Propagation of Shock Waves in Inhomogeneous Gases. VI : Oblique Hydromagnetic Shock Propagation
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概要
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The propagation of a hydromagnetic fast shock in a gravitational atmosphere permeated by a uniform magnetic field is studied by means of generalized Chisnell's method. It is shown that the fast shock propagating upwards always refracts away from the vertical irrespective of the direction of the magnetic field and the degree of refraction is higher when the ratio of the sound velocity to the Alfven velocity along the magnetic field is smaller than unity. It is also shown that slow waves travelling upwards and downwards are generated in the fast-shock propagation through the atmosphere of declining density. The relation between these results and the heating of the solar corona is discussed.
- 理論物理学刊行会の論文
- 1969-02-25
著者
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HASHIMOTO Yoshiaki
Department of Electric and Electronic Engineering, Toyohashi University of Technology
-
ONO Yoro
Department of Physics, Hokkaido University
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Ono Yoro
Department Of Physics Hokkaido University
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Yamazaki Hatuo
Department Of Nuclear Engineering Hokkaido University
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HASHIMOTO Yoshiaki
Department of Physics, Hirosaki University
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