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Showing 1 to 7 of 7 for “"rotating fluids"”.
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Thermal Convection in Rotating Fluids
Made available in DSpace on 2014-12-10T21:24:53Z (GMT). No. of bitstreams: 1 7500248.pdf: 6750417 bytes, checksum: 075f78830a9cd65237def3a561df8f77 (MD5) Previous issue date: 1974
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The role of viscosity in stratified rotating fluids
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Meteorology, 1964.
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Centrifugally Driven Thermal Convection and Gravitational Instabilities in Bounded Rotating Fluids
Made available in DSpace on 2014-12-08T23:18:29Z (GMT). No. of bitstreams: 1 7013353.pdf: 8219439 bytes, checksum: f8ec41ed52b8b72a178246af8b87dde0 (MD5) Previous issue date: 1969
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Contributions to the study of shear-free and of purely radiative perfect fluids in general relativity
A study of shear-free perfect fluids in general relativity (rotating and/or expanding) and a characterisation of the orthogonal Bianchi class A perfect fluids as geodesic, non-rotating fluids with vanishing divergence of the electric and magnetic part of the Weyl tensor.
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LONG TIME BEHAVIOR OF LINEAR AND NONLINEAR WAVES:LARGE LARGE AMPLITUDE TRAVELING QUASI-PERIODIC SOLUTIONS IN FLUID MECHANICS AND DYNAMICS OF LINEAR WAVE EQUATIONS
… (MHD) system and the 2D-Euler equation for rotating fluids ($\beta$-plane equation), both in presence of a large amplitude traveling wave external force with large velocity speed $\lambda \omega$, where $\lambda \gg 1$ is a large parameter. For both equations we prove the existence of large …
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Helical waves in Earth's outer core
… is greater than $0.1$. Separately, in the rotating turbulence literature, there is preliminary evidence of a similarly sharp transition from a columnar flow structure to incoherent turbulence when the Rossby number is $ Ro \sim 0.2-0.6$. We show, that when $Ro > Ro^{\text{crit}} \approx …