On oscillatory Marangoni convection in rotating fluid layer with flat free surface subject to uniform heat flux from below |
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| Affiliation: | 1. Institute of Geophysics, ETH Zürich, Sonneggstrasse 5, CH-8092 Zürich, Switzerland;2. Institute of Geology, ETH Zürich, Sonneggstrasse 5, CH-8092, Zürich, Switzerland;4. Geo Explorers International Ltd, Schlossstrasse 3, CH-4133 Pratteln, Switzerland;5. Geoscience Centre of the University of Göttingen, Goldschmidtstr. 3, 37077 Göttingen, Germany;1. Department of Tectonics and Sedimentology, Freie Universität Berlin, Malteserstraße 74-100, 12449 Berlin, Germany;2. Sorbonne Universités, UPMC Univ Paris 06, UMR 7193, iSteP, F-75005 Paris, France;3. CNRS, UMR 7193, ISTeP, F-75005, Paris, France 05 PARIS, France;1. Université de Lyon, Université Jean Monnet, UMR CNRS IRD 6524, Laboratoire Magmas et Volcans, 42023 Saint Etienne, France;2. Microstructures and Processing Department, Ecole nationale supérieure des mines de Saint-Etienne, 158 cours Fauriel, 42023 Saint-Etienne, France;3. Department of Earth Sciences, Durham University, Science Labs, Durham DH1 3LE, England, United Kingdom;1. CEA, DAM, DIF, F-91297 Arpajon, France;2. Laboratoire de Géologie, Ecole Normale Supérieure/CNRS UMR 8538, PSL Research University, Paris 75005, France;3. Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, UMR 7154 CNRS, Paris, France;4. Department of Mines and Geology, National Seismological Center, Kathmandu, Nepal |
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| Abstract: | The effect of uniform rotation on the onset of steady and oscillatory surface-tension-driven (Marangoni) convection in a horizontal fluid layer with a flat free upper surface and heated from below with a uniform heat flux is considered theoretically using linear stability theory. The Ta–Pr parameter space, divided into domains in which either steady or oscillatory convection is preferred, is presented. |
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