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<div class="definition"><div class="short_definition">(<br/>''Also called'' [[hydrostatic stability]], [[vertical stability]].) The ability of a fluid at rest  to become turbulent or laminar due to the effects of [[buoyancy]].</div><br/> <div class="paragraph">A fluid, such as air, tending to become or remain turbulent is said to be statically unstable; one  tending to become or remain laminar is statically stable; and one on the borderline between the  two (which might remain laminar or turbulent depending on its history) is statically neutral. The  concept of static stability can also be applied to air not at rest by considering only the buoyant  effects and neglecting all other [[shear]] and inertial effects of motion. However, if any of these other  [[dynamic stability]] effects would indicate that the flow is dynamically unstable, then the flow will  become turbulent regardless of the static stability. That is, [[turbulence]] has physical priority, when  considering all possible measures of flow [[stability]] (e.g., the air is turbulent if any one or more of  static, dynamic, inertial, [[barotropic]], etc., effects indicates [[instability]]). Turbulence that forms in  statically [[unstable air]] will act to reduce or eliminate the instability that caused it by moving less  dense fluid up and more dense fluid down, and by creating a neutrally buoyant mixture. Thus,  turbulence will tend to decay with time as static instabilities are eliminated, unless some outside  forcing (such as heating of the bottom of a layer of air by contact with the warm ground during  a sunny day) continually acts to destabilize the air. This latter mechanism is one of the reasons  why the [[atmospheric boundary layer]] can be turbulent all day. <br/>''Compare'' [[dynamic stability]], [[lapse  rate]], [[Brunt&ndash;V&auml;is&auml;l&auml; frequency]], [[nonlocal static stability]], [[adiabatic equilibrium]]; <br/>''see also'' [[slice  method]], [[buoyant instability]]</div><br/> </div><div class="reference">Stull, R. B. 1991. Static stability&mdash;An update. Bull. Amer. Meteor. Soc.. 72. 1521&ndash;1529. </div><br/>  
<div class="definition"><div class="short_definition">(''Also called'' [[hydrostatic stability]], [[vertical stability]].) The ability of a fluid at rest  to become turbulent or laminar due to the effects of [[buoyancy]].</div><br/> <div class="paragraph">A fluid, such as air, tending to become or remain turbulent is said to be statically unstable; one  tending to become or remain laminar is statically stable; and one on the borderline between the  two (which might remain laminar or turbulent depending on its history) is statically neutral. The  concept of static stability can also be applied to air not at rest by considering only the buoyant  effects and neglecting all other [[shear]] and inertial effects of motion. However, if any of these other  [[dynamic stability]] effects would indicate that the flow is dynamically unstable, then the flow will  become turbulent regardless of the static stability. That is, [[turbulence]] has physical priority, when  considering all possible measures of flow [[stability]] (e.g., the air is turbulent if any one or more of  static, dynamic, inertial, [[barotropic]], etc., effects indicates [[instability]]). Turbulence that forms in  statically [[unstable air]] will act to reduce or eliminate the instability that caused it by moving less  dense fluid up and more dense fluid down, and by creating a neutrally buoyant mixture. Thus,  turbulence will tend to decay with time as static instabilities are eliminated, unless some outside  forcing (such as heating of the bottom of a layer of air by contact with the warm ground during  a sunny day) continually acts to destabilize the air. This latter mechanism is one of the reasons  why the [[atmospheric boundary layer]] can be turbulent all day. <br/>''Compare'' [[dynamic stability]], [[lapse rate|lapse  rate]], [[Brunt&ndash;V&#x000e4;is&#x000e4;l&#x000e4; frequency]], [[nonlocal static stability]], [[adiabatic equilibrium]]; <br/>''see also'' [[slice method|slice  method]], [[buoyant instability]]</div><br/> </div><div class="reference">Stull, R. B. 1991. Static stability&mdash;An update. Bull. Amer. Meteor. Soc.. 72. 1521&ndash;1529. </div><br/>  
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Latest revision as of 16:58, 25 April 2012



static stability

(Also called hydrostatic stability, vertical stability.) The ability of a fluid at rest to become turbulent or laminar due to the effects of buoyancy.

A fluid, such as air, tending to become or remain turbulent is said to be statically unstable; one tending to become or remain laminar is statically stable; and one on the borderline between the two (which might remain laminar or turbulent depending on its history) is statically neutral. The concept of static stability can also be applied to air not at rest by considering only the buoyant effects and neglecting all other shear and inertial effects of motion. However, if any of these other dynamic stability effects would indicate that the flow is dynamically unstable, then the flow will become turbulent regardless of the static stability. That is, turbulence has physical priority, when considering all possible measures of flow stability (e.g., the air is turbulent if any one or more of static, dynamic, inertial, barotropic, etc., effects indicates instability). Turbulence that forms in statically unstable air will act to reduce or eliminate the instability that caused it by moving less dense fluid up and more dense fluid down, and by creating a neutrally buoyant mixture. Thus, turbulence will tend to decay with time as static instabilities are eliminated, unless some outside forcing (such as heating of the bottom of a layer of air by contact with the warm ground during a sunny day) continually acts to destabilize the air. This latter mechanism is one of the reasons why the atmospheric boundary layer can be turbulent all day.
Compare dynamic stability, lapse rate, Brunt–Väisälä frequency, nonlocal static stability, adiabatic equilibrium;
see also slice method, buoyant instability

Stull, R. B. 1991. Static stability—An update. Bull. Amer. Meteor. Soc.. 72. 1521–1529.


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