Rayleigh-Taylor instability of a two-fluid layer under a general rotation field and horizontal magnetic field

DOI10.1007/BF00644702zbMath0941.76031OpenAlexW2055010118MaRDI QIDQ1370883

L. A. Dávalos-Orozco

Publication date: 7 August 2000

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00644702

zbMATH Keywords

rotationRayleigh-Taylor instabilitytravelling wavetwo-layer fluidhydromagnetic stabilityuniform horizontal magnetic fieldUranusstability of planetary interiors

Mathematics Subject Classification ID

Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Rotation in hydrodynamic stability (76E07) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (4)

Rayleigh-Taylor and Richtmyer-Meshkov instability induced flow, turbulence, and mixing. II ⋮ Cylindrical rotating Rayleigh–Taylor instability ⋮ Effects of general rotation and a horizontal magnetic field on the Rayleigh-Taylor instability of three-fluid layer in porous media ⋮ Rayleigh-Taylor instability with general rotation and surface tension in porous media

Cites Work

• Unnamed Item
• Rayleigh–Taylor instability of a continuously stratified magnetofluid under a general rotation field
• Rayleigh–Taylor instability of a continuously stratified fluid under a general rotation field

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