Rayleigh–Bénard and schwarzschild instability in a supercritical fluid
Due to the density stratification, the convection onset criterion in a supercritical fluid layer heated from below includes a stabilizing effect known as the Schwarzschild criterion, which requires an adaptation of the classical low Mach number approximation. We numerically solve the mathematical mo...
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Published in: | Advances in space research Vol. 36; no. 1; pp. 11 - 16 |
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Main Authors: | , , , |
Format: | Journal Article |
Language: | English |
Published: |
Elsevier Ltd
2005
Elsevier |
Subjects: | |
Online Access: | Get full text |
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Summary: | Due to the density stratification, the convection onset criterion in a supercritical fluid layer heated from below includes a stabilizing effect known as the Schwarzschild criterion, which requires an adaptation of the classical low Mach number approximation. We numerically solve the mathematical model describing the motion of a supercritical fluid in the classical Rayleigh–Bénard configuration and we bring to the fore two main events: (i) the reverse transition of an unstable layer to stability without any external intervention; (ii) the convection onset according to the Schwarzschild criterion. In addition, the 3D extension of the study is briefly described. |
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ISSN: | 0273-1177 1879-1948 |
DOI: | 10.1016/j.asr.2005.02.082 |