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10.1038/srep11706 http://scihub22266oqcxt.onion/10.1038/srep11706 C4486928!4486928!26130005     free     free     free Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Sci+Rep 2015 ; 5 (ä): ä Nephropedia Template TP {{tp|p=26130005|t=2015. The Inhibition of the Rayleigh-Taylor Instability by Rotation |pdf=|usr=}}{{26130005}} gab.com Text The Inhibition of the Rayleigh-Taylor Instability by Rotation JO: Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=26130005 #FOAvip It is well-established that the Coriolis force that acts on fluid in a rotating system can act to stabilise otherwise unstable flows. Chandrasekhar considered theoretically the effect of the Coriolis force on the Rayleigh-Taylor instability, which occurs at the interface between a dense fluid lying on top of a lighter fluid under gravity, concluding that rotation alone could not stabilise this system indefinitely. Recent numerical work suggests that rotation may, nevertheless, slow the growth of the instability. Experimental verification of these results using standard techniques is problematic, owing to the practical difficulty in establishing the initial conditions. Here, we present a new experimental technique for studying the Rayleigh-Taylor instability under rotation that side-steps the problems encountered with standard techniques by using a strong magnetic field to destabilize an otherwise stable system. We find that rotation about an axis normal to the interface acts to retard the growth rate of the instability and stabilise long wavelength modes; the scale of the observed structures decreases with increasing rotation rate, asymptoting to a minimum wavelength controlled by viscosity. We present a critical rotation rate, dependent on Atwood number and the aspect ratio of the system, for stabilising the most unstable mode. Twit Text FOAVip The Inhibition of the Rayleigh-Taylor Instability by Rotation ????Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=26130005 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=26130005 #FOAvip English Wikipedia <ref>{{Cite pmid|26130005}}</ref> The Inhibition of the Rayleigh-Taylor Instability by Rotation #MMPMID26130005 Baldwin KA; Scase MM; Hill RJA Sci Rep 2015[]; 5 (ä): ä PMID26130005show ga It is well-established that the Coriolis force that acts on fluid in a rotating system can act to stabilise otherwise unstable flows. Chandrasekhar considered theoretically the effect of the Coriolis force on the Rayleigh-Taylor instability, which occurs at the interface between a dense fluid lying on top of a lighter fluid under gravity, concluding that rotation alone could not stabilise this system indefinitely. Recent numerical work suggests that rotation may, nevertheless, slow the growth of the instability. Experimental verification of these results using standard techniques is problematic, owing to the practical difficulty in establishing the initial conditions. Here, we present a new experimental technique for studying the Rayleigh-Taylor instability under rotation that side-steps the problems encountered with standard techniques by using a strong magnetic field to destabilize an otherwise stable system. We find that rotation about an axis normal to the interface acts to retard the growth rate of the instability and stabilise long wavelength modes; the scale of the observed structures decreases with increasing rotation rate, asymptoting to a minimum wavelength controlled by viscosity. We present a critical rotation rate, dependent on Atwood number and the aspect ratio of the system, for stabilising the most unstable mode. äThe Inhibition of the Rayleigh-Taylor Instability by Rotation (epmc).pdf DeepDyve Pubget Overpricing