Abstract
The modes of thermovibrational convection in square cavity with rigid boundaries under microgravity conditions are investigated. The cavity undergoes linearly polarized high-frequency vibrations in the direction parallel to the gravitational field. External temperature gradient is perpendicular to the vibration direction. The parameter V proportional to the ratio of the vibration acceleration to the gravity acceleration and independent of the temperature difference has been chosen as a dimensionless parameter characterizing the vibration intensity. The map of convection modes in the parameter plane Grashof number – vibration parameter and the boundary of stationary average convection stability have been obtained. It is found that depending on the values of the vibration parameter and Grashof number, one-, three- or four-vortex stationary modes of convection can be realized. When the Gr number increases, the stationary average motion becomes unstable and oscillatory convection modes arise.
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This article belongs to the Topical Collection: The effect of gravity on non-equilibrium processes in fluids
Guest Editors: Tatyana Lyubimova, Valentina Shevtsova
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Perminov, A.V., Nikulina, S.A. & Lyubimova, T.P. Analysis of Thermovibrational Convection Modes in Square Cavity Under Microgravity Conditions. Microgravity Sci. Technol. 34, 34 (2022). https://doi.org/10.1007/s12217-022-09956-1
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DOI: https://doi.org/10.1007/s12217-022-09956-1