Effect of Hall current and resistivity on the stability of a gas–liquid system

1970/09/01 by G. L. Kalra, S. N. Kathuria, R. J. Hosking +1
Physics and Astronomy · Biochemistry, Genetics and Molecular Biology · #Solar and Space Plasma Dynamics #Ionosphere and magnetosphere dynamics #Geomagnetism and Paleomagnetism Studies

paper · doi:10.1017/s0022377800005158

Abstract

The stability of a non-conducting, compressible fluid (gas) flowing across the surface of incompressible conducting fluid (liquid) is discussed. Finite resistivity and Hall current are included in the hydromagnetic equations, together with surface tension. Both subsonic and supersonic flows are treated and some new instabilities are found, together with modifications to real and oscillatory modes obtained in earlier treatments.

Citations

• Investigation of the Kelvin-Helmholtz Instability in a Cesium Plasma

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