Issue |
EAS Publications Series
Volume 82, 2019
Astro Fluid: An International Conference in Memory of Professor Jean-Paul Zahn's Great Scientific Achievements
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Page(s) | 259 - 269 | |
Section | Seismology and Stellar Structure, Evolution and Rotation | |
DOI | https://doi.org/10.1051/eas/1982026 | |
Published online | 21 June 2019 |
A.S. Brun, S. Mathis, C. Charbonnel and B. Dubrulle (eds)
EAS Publications Series, 82 (2019) 259-269
Mean flow evolution of saturated forced shear flows in polytropic atmospheres
Department of Mathematics, City University of London, Northampton Square, London, EC1V 0HB, UK
In stellar interiors shear flows play an important role in many physical processes. So far helioseismology provides only large-scale measurements, and so the small-scale dynamics remains insufficiently understood. To draw a connection between observations and three-dimensional DNS of shear driven turbulence, we investigate horizontally averaged profiles of the numerically obtained mean state. We focus here on just one of the possible methods that can maintain a shear flow, namely the average relaxation method. We show that although some systems saturate by restoring linear marginal stability this is not a general trend. Finally, we discuss the reason that the results are more complex than expected.
© EAS, EDP Sciences, 2019