Moreover, the squeezing of gases can convert smooth, grape-like shapes into wrinkled raisins _ a phenomenon called Rayleigh-Taylor instability _ which also drastically reduces fusion yields.
12.
The bubble becomes less of a sphere and looks more like the Crab Nebula, the deviation of which from a smooth surface is also due to Rayleigh Taylor instability.
13.
Likewise, in various systems and geometries, when the Taylor number exceeds a critical value, inertial instabilities set in, sometimes known as Taylor instabilities, which may lead to Taylor vortices or cells.
14.
Once the overlying layers have become denser, the weak salt layer will tend to deform into a characteristic series of ridges and depressions, due to a form of Rayleigh Taylor instability.
15.
This led to hot spots on the pellet which were imprinted into the imploding plasma, seeding Rayleigh Taylor instabilities and thereby mixing the plasma so the center did not collapse uniformly.
16.
Beam timing is a relatively simple issue though and is solved by using Rayleigh Taylor instabilities in the fuel, prematurely mixing it and reducing heating efficacy at the time of maximum compression.
17.
If you enjoy analyzing things numerically, you can look at the empirical laws we use to model convective instability-like a Rayleigh-Taylor instability model . talk ) 14 : 46, 28 July 2012 ( UTC)
18.
If you left it long enough for the jam to fall on its own, the process by which the jam breaks through the air holding it up is the Rayleigh Taylor instability .-- talk ) 17 : 52, 28 November 2011 ( UTC)
19.
Dr . Marc W . Pound of the University of Maryland said the the observations revealed velocities and densities of matter flowing from the bottom to the tip of the cloud columns were " inconsistent with those expected from the Rayleigh-Taylor instability ."
20.
Geophysicists believe that hotspots originate at one of two major boundaries deep in the Earth, either a shallow interface in the lower viscous portion of the upper layer would become less dense due to thermal expansion, and rise towards the surface as a Rayleigh-Taylor instability.
