Internal rotation in stars ( Ogilvie, 2007 ), and even planetary dynamos ( Petitdemange et al ., 2008 ) may, under some circumstances, be vulnerable to the MRI in combination with convective instabilities.
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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)
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Convective instability is also termed " static instability ", because the instability does not depend on the existing motion of the air; this contrasts with dynamic instability where instability is dependent on the motion of air and its associated effects such as dynamic lifting.
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Or, the wind gusts may be produced by a dry cold front, that is, a cold front that is moving into a dry air mass and is producing no convective instability resulting from cooler air riding over heated ground can maintain the dust storm initiated at the front.
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By considering modes with zero group velocity and determining whether they grow or decay, we can determine whether an initial condition which is localised around x = 0 moves away from x = 0 as it grows, with y ( 0, t ) \ rightarrow 0 ( convective instability ); or whether y ( 0, t ) \ rightarrow \ infty ( absolute instability ).
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B . A . Finlayson first explained in 1970 ( in his paper " Convective instability of ferromagnetic fluids ", " Journal of Fluid Mechanics ", "'40 "': 753-767 ) how an external magnetic field imposed on a ferrofluid with varying magnetic susceptibility, e . g ., due to a temperature gradient, results in a nonuniform magnetic body force, which leads to "'thermomagnetic convection " '.
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