hydromagnetic

This was followed by sustained work on hydrodynamic and hydromagnetic stability from 1950 to 1961.

A mathematical description of peristaltic hydromagnetic flow in a tube.

Models with closed gate B are called hydromagnetic dynamos.

When the HydroMagnetic water coaster opened, it operated with ten 6-passenger boats.

Finally, a hydromagnetic dynamo process in the polar regions of the inner magnetosphere may be possible.

On April 13, 2012 it was announced the first 6-man Tornado would built using Hydromagnetic technology.

Waves with frequencies smaller than the gyrofrequency are called hydromagnetic waves.

The concept is useful in solar dynamics and in hydromagnetic dynamo theory.

An oscillating hydromagnetic non-Newtonian flow in a rotating system.

Alfvén waves (low frequency hydromagnetic plasma oscillations) are named in his honor.

Bootlegger's Run - a water roller coaster featuring new generation hydromagnetic technology (opening in 2013 season)

Virtually all dynamos in astrophysics and geophysics are hydromagnetic dynamos.

"Stimulated Compton scattering of hydromagnetic waves in the interstellar medium", Astrophys.

These were originally interpreted as hydromagnetic waves, but on later analysis it was realized that they were due to field-aligned or Birkeland currents.

Hydrodynamic and Hydromagnetic Stability (Dover).

Powered by a hydromagnetic dynamo process driven by the inductive action of internal solar flows, the solar cycle:

In 2010, ProSlide announced that they would be combining the family rafting and water coaster technologies to create a Hydromagnetic Mammoth.

Because the phase velocity of the magnetosonic mode is almost always larger than v, the magnetosonic wave is often called the "fast" hydromagnetic wave.

Riven fragments of atoms sleeted through vacuum, were whirled away by the ship's hydromagnetic field, spat X-rays into her material shielding and vanished starward.

In the hydromagnetic model, the current reaches an upper limit, similar to a technical dynamo during short circuit, while the wind amplitude breaks down to a fraction of its original value.

Hydrodynamic and hydromagnetic stability, Chandrasekhar, Subrahmanyan; International Series of Monographs on Physics, Oxford: Clarendon, 1961, p. 622.

The MRI was first noticed in a non-astrophysical context by Evgeny Velikhov in 1959 when considering the stability of Couette flow of an ideal hydromagnetic fluid.

His Ph.D. dissertation, entitled "Hydromagnetic Equilibrium of a Fluid Sphere" and supervised by Subrahmanyan Chandrasekhar, was split into three separate papers and published in The Astrophysical Journal in 1963 and 1964.