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Conditional symmetric instability

Conditional symmetric instability, or CSI, is a form of convective instability in a fluid subject to temperature differences in a uniform rotation frame of reference while it is thermally stable in the vertical and dynamically in the horizontal. The instability in this case develop only in an inclined plane with respect to the two axes mentioned and that is why it can give rise to a so-called "slantwise convection" if the air parcel is almost saturated and moved laterally and vertically in a CSI area. This concept is mainly used in meteorology to explain the mesoscale formation of intense precipitation bands in an otherwise stable region, such as in front of a warm front. The same phenomenon is also applicable to oceanography.

Principle
Hydrostatic stability (in red) and dew point (in green) on a Skew-T log-P diagram. An air particle at a certain altitude will be stable if its adiabatically modified temperature during an ascent is equal to or cooler than the environment. Similarly, it is stable if its temperature is equal or warmer during a descent. In the case where the temperature is equal, the particle will remain at the new altitude, while in the other cases, it will return to its initial level4. In the diagram on the right, the yellow line represents a raised particle whose temperature remains at first under that of the environment (stable air) which entails no convection. Then in the animation, there is warming surface warming and the raised particle remains warmer than the environment (unstable air). A measure of hydrostatic stability is to record the variation with the vertical of the equivalent potential temperature (\theta_e): ::* If \theta_e diminish with altitude leads to unstable airmass ::* If \theta_e remains the same with altitude leads to neutral airmass ::* If \theta_e increase with altitude leads to stable airmass. Inertial stability In the same way, a lateral displacement of an air particle changes its absolute vorticity \eta. This is given by the sum of the planetary vorticity, f, and \zeta, the geostrophic (or relative) vorticity of the parcel: {{center|\eta= \left[ \frac{\partial v}{\partial x} - \frac{\partial u}{\partial y} \right ] + f = \zeta + f \qquad \qquad }} Where : • v and u are the meridional and zonal geostrophic velocities respectively. • x and y correspond to the zonal and meridional coordinates. • f is the Coriolis parameter, which describes the component of vorticity around the local vertical that results from the rotation of the reference frame. • \zeta is the relative vorticity around the local vertical. It is found by taking the vertical component of the curl of the geostrophic velocity. \eta can be positive, null or negative depending on the conditions in which the move is made. As the absolute vortex is almost always positive on the synoptic scale, one can consider that the atmosphere is generally stable for lateral movement. Inertial stability is low only when \eta is close to zero. Since f is always positive, \eta \le 0 can be satisfied only on the anticyclonic side of a strong maximum of jet stream or in a barometric ridge at altitude, where the derivative velocities in the direction of displacement in the equation give a significant negative value. • \Delta M_g = 0 , the particle then remains at the new position because its momentum has not changed • \Delta M_g > 0 , the particle returns to its original position because its momentum is greater than that of the environment • \Delta M_g , the particle continues its displacement because its momentum is smaller than that of the environment. Slantwise movement Under certain stable hydrostatic and inertial conditions, slantwise displacement may, however, be unstable when the particle changes air mass or wind regime. The figure on the right shows such a situation. The displacement of the air particle is done with respect to kinetic moment lines (\scriptstyle M_g) that increase from left to right and equivalent potential temperature (\scriptstyle \theta_e) that increase with height. ;Lateral movement A Horizontal accelerations (to the left or right of a surface \scriptstyle M_g ) are due to an increase/decrease in the \scriptstyle M_g of the environment in which the particle moves. In these cases, the particle accelerates or slows down to adjust to its new environment. Particule A undergoes a horizontal acceleration that gives it positive buoyancy as it moves to colder air and decelerates as it moves to a region of smaller \scriptstyle M_g . The particle rises and eventually becomes colder than its new environment. At this point, it has negative buoyancy and begins to descend. In doing so, \scriptstyle M_g increases and the particle returns to its original position. ;Vertical displacement B Vertical movements in this case result in negative buoyancy as the particle encounters warmer air ( \scriptstyle \theta_e increases with height) and horizontal acceleration as it moves to larger surfaces \scriptstyle M_g . As the particle goes down, its \scriptstyle M_g decreases to fit the environment and the particle returns to B. ; Slantwise displacement C Only case C is unstable. Horizontal acceleration combines with a vertical upward disturbance and allows oblique displacement. Indeed, the \scriptstyle \theta_e of the particle is larger than the \scriptstyle \theta_e of the environment. While the momentum of the particle is less than that of the environment. An oblique displacement thus produces a positive buoyancy and an acceleration in the oblique displacement direction which reinforces it. The condition for having conditional symmetric instability in an otherwise stable situation is therefore that: • the slope of \scriptstyle \theta_e is greater than that of \scriptstyle M_g • Laterally displaced air is almost saturated. ==Potential effects==
Potential effects
CSI is usually embedded in large areas of vertical upward motion. The ideal situation is a geostrophic flow from the South with wind speeds that increase with height. The environment is well mixed and close to saturation. Since the flow is unidirectional, the u component of the wind can be set equal to zero, which establishes a symmetrical flow perpendicular to the temperature gradient in the air mass. This type of flow is typically found in baroclinic atmospheres with cold air to the west. Conditional symmetric instability affects a layer that can be thin or very large in the vertical, similar to hydrostatic convection. The thickness of the layer determines the enhancement of convective precipitation within a region otherwise stratiform clouds. ==References==
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