Sentences with phrase «conserve angular»

In a vortex, turbulence is inhibited because when a particle of air moves inward, its tangential velocity increases to conserve angular momentum.
The density will continue to increase without limit, as the gravitational force increases due to the inverse square law of gravity, and the rotation will speed up, to conserve the angular momentum of the initial state, as the size decreases, so the moment of inertia continues to decline, and angular velocity increases to keep I. omega ^ 2 constant.
If a skater is spinning with out - stretched arms and they pull their arms closer into their body, the skater will begin to spin faster in order to conserve angular momentum.
Since the 4 ms slowdown over 30 years was followed by a similar but slightly reduced speedup over the next 30 years, it is clear that a lot of the energy difference needed to conserve angular momentum had to have been stored elastically in the mantle rather than being dissipated to viscous heating of the mantle.
Basic physics tells us that as the diameter increases, the rate of rotation will slow in order to conserve angular momentum.
4) I say that when air moves from a location with high rotational velocity (m / s following a circumference) to a location with a low angular velocity, the air will conserve angular momentum and hence be diverted at right angles to the the initial impetus, resulting (at the poles) in a vortex around the pole.
For instance, if the winds that whip around the planet slow down, the Earth spins faster to conserve angular momentum.
For spirals, on the other hand, the gas infelt slowly conserving its angular momentum and stars formed steadily along a timescale comparable to the age of the Universe.
That's because the recipe exploits the fact that the black hole conserves angular momentum, so that its final spin is equal to its initial spin plus that of the electron.
If you know of a mechanism whereby the Moon might be captured into a geocentric orbit whilst conserving angular momentum, please do let everyone know.
Our planet as a whole conserves its angular momentum except for the known effects of external torque associated with the lunar - solar tide, which induces a gradual decelerating of the earth rotation velocity at a rate corresponding to the increase in the astronomic length of day (LOD) by about 1.4 millisecond per century (Munk and McDonald 1960).
As it is, a Hadley cell that conserves angular momentum develops large wind shears and the flow becomes baroclinically unstable (it can be shown through the so - called thermal wind equation that the vertical gradient of the horizontal wind velocity is proportional to the horizontal temperature gradient).

Not exact matches

At that time, a problem arose because it seemed that both energy and angular momentum were not conserved in beta - decay.
The spin of such cosmic objects is described by a conserved quantity called angular momentum, which accounts for both the speed of the rotating mass and its distance from the spin axis.
The complete quote is «Were angular momentum conserved this would lead to ridiculous spin rates, so it has long been known that angular momentum must be lost» -LRB-!)
We do know both mechanical energy and angular momentum are conserved quantities in any setup (with no dissipative processes, of course).
Also with angular momentum being conserved, it must fall.
The requirement that both energy and angular momentum are conserved means that there's an unique connection between the rate of exchange of angular momentum and the rate of dissipation.
Basically, I am aware that the model differencing schemes are specifically designed to conserve, mass, energy, linear and angular momentum, and vorticity.
In the so - called model numerics, a great deal of care is used in formulating the differential equation solution approach so as to explicitly conserve a number of quantities (mass, energy, water substance, angular momentum, linear momentum, vorticity) that are all important for the accurate representation of atmospheric dynamics.
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