Dynamic stabilisation of Rayleigh-Taylor instability

Details Dynamic stabilisation of Rayleigh-Taylor instability Dynamic stabilisation of Rayleigh-Taylor instability

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..88..255s&link_type=abstract

Astrophysics and Space Science, vol. 88, no. 1, Nov. 1982, p. 255-259.

Astronomy and Astrophysics

Astrophysics

1

Dynamic Stability, Flow Stability, Magnetic Fields, Oscillating Flow, Stratified Flow, Taylor Instability, Gravitational Effects, Hydrodynamic Equations, Incompressible Fluids, Inviscid Flow, Mathieu Function

Scientific paper

A vertically oscillating system consisting of a stratified fluid whose density increases exponentially upward, and is subjected to a gravitational field acting downward, has residual instabilities associated with disturbances of small wavelengths in the vertical direction that may be removed by the application of a vertical magnetic field. This demonstrates that the vertical magnetic field, when applied to a vertically oscillating system to which a degree of electrical conductivity is imparted, can stabilize the latter with respect to small-wavelength disturbances in the vertical direction.

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