THE CHARACTER OF THE EQUILIBRIUM OF A HEAVY, VISCOUS, INCOMPRESSIBLE, ROTATING FLUID OF VARIABLE DENSITY
From MaRDI portal
Publication:3240032
DOI10.1093/QJMAM/9.1.22zbMath0074.42403OpenAlexW2080302113MaRDI QIDQ3240032
Publication date: 1956
Published in: The Quarterly Journal of Mechanics and Applied Mathematics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1093/qjmam/9.1.22
Related Items (11)
On the magnetism of stars and planets ⋮ Analysis of Rayleigh Taylor instability in nanofluids with rotation ⋮ Centrifugally forced Rayleigh–Taylor instability ⋮ Analysis of magnetized Rayleigh-Taylor instability in nanofluids through porous medium ⋮ Rayleigh-Taylor and Richtmyer-Meshkov instability induced flow, turbulence, and mixing. II ⋮ Hydromagnetic Flow due to an Oscillating Plane ⋮ Rayleigh–Taylor instability of a continuously stratified fluid under a general rotation field ⋮ 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 ⋮ Nonradial stellar oscillations excited by turbulent convection ⋮ Rotating rayleigh-taylor instability as a model of sinking events in the ocean
This page was built for publication: THE CHARACTER OF THE EQUILIBRIUM OF A HEAVY, VISCOUS, INCOMPRESSIBLE, ROTATING FLUID OF VARIABLE DENSITY
