Rayleigh-Taylor stability in the presence of rotation

Details Rayleigh-Taylor stability in the presence of rotation Rayleigh-Taylor stability in the presence of rotation

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.175..149o&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 175, no. 1, Jan. 1991, p. 149-155.

Computer Science

Numerical Analysis

1

Density (Mass/Volume), Incompressible Fluids, Rotating Fluids, Taylor Instability, Boundary Conditions, Numerical Analysis, Perturbation

Scientific paper

The stability of a slab of incompressible fluid with exponentially-increasing density, supported by a semi-infinite homogeneous region and supporting a semi-infinite region of exponentially-decreasing density has been investigated when the whole system rotates uniformly about a vertical axis. The familiar Reyleigh-Taylor stability problems are recovered from the general dispersion relation, both in the presence of rotation and in the absence of rotation.

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