Shear production: Difference between revisions

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<div class="definition"><div class="short_definition">The generation of [[turbulence kinetic energy]] caused by [[wind shear]].</div><br/> <div class="paragraph">This mechanical production term ''S'' of the turbulence kinetic energy budget equation is (written  in [[Einstein's summation notation]])  <div class="display-formula"><blockquote>[[File:ams2001glos-Se20.gif|link=|center|ams2001glos-Se20]]</blockquote></div> and is almost always positive, that is, a source. In the fair-weather, turbulent [[atmospheric boundary  layer]], the terms associated with horizontal wind usually dominate, allowing the shear production  term to be approximated as  <div class="display-formula"><blockquote>[[File:ams2001glos-Se21.gif|link=|center|ams2001glos-Se21]]</blockquote></div> where (<div class="inline-formula">[[File:ams2001glos-Sex03.gif|link=|ams2001glos-Sex03]]</div>,<div class="inline-formula">[[File:ams2001glos-Sex04.gif|link=|ams2001glos-Sex04]]</div>) are the [[Reynolds stresses]] (turbulent kinematic [[momentum fluxes]]) in the  (''x'', ''y'') directions, (''U'', ''V'') are the respective wind components, the prime denotes [[deviation]] from  the mean, and the overbar denotes an average. The ratio of the buoyant to the negative of the  shear production terms is also known as the [[flux Richardson number]] and is a measure of [[dynamic  stability]].</div><br/> </div>
<div class="definition"><div class="short_definition">The generation of [[turbulence kinetic energy]] caused by [[wind shear]].</div><br/> <div class="paragraph">This mechanical production term ''S'' of the turbulence kinetic energy budget equation is (written  in [[Einstein's summation notation]])  <div class="display-formula"><blockquote>[[File:ams2001glos-Se20.gif|link=|center|ams2001glos-Se20]]</blockquote></div> and is almost always positive, that is, a source. In the fair-weather, turbulent [[atmospheric boundary layer|atmospheric boundary  layer]], the terms associated with horizontal wind usually dominate, allowing the shear production  term to be approximated as  <div class="display-formula"><blockquote>[[File:ams2001glos-Se21.gif|link=|center|ams2001glos-Se21]]</blockquote></div> where (<div class="inline-formula">[[File:ams2001glos-Sex03.gif|link=|ams2001glos-Sex03]]</div>,<div class="inline-formula">[[File:ams2001glos-Sex04.gif|link=|ams2001glos-Sex04]]</div>) are the [[Reynolds stresses]] (turbulent kinematic [[momentum flux|momentum fluxes]]) in the  (''x'', ''y'') directions, (''U'', ''V'') are the respective wind components, the prime denotes [[deviation]] from  the mean, and the overbar denotes an average. The ratio of the buoyant to the negative of the  shear production terms is also known as the [[flux Richardson number]] and is a measure of [[dynamic stability|dynamic  stability]].</div><br/> </div>
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Latest revision as of 16:52, 25 April 2012



shear production

The generation of turbulence kinetic energy caused by wind shear.

This mechanical production term S of the turbulence kinetic energy budget equation is (written in Einstein's summation notation)
ams2001glos-Se20
and is almost always positive, that is, a source. In the fair-weather, turbulent atmospheric boundary layer, the terms associated with horizontal wind usually dominate, allowing the shear production term to be approximated as
ams2001glos-Se21
where (
ams2001glos-Sex03
,
ams2001glos-Sex04
) are the Reynolds stresses (turbulent kinematic momentum fluxes) in the (x, y) directions, (U, V) are the respective wind components, the prime denotes deviation from the mean, and the overbar denotes an average. The ratio of the buoyant to the negative of the shear production terms is also known as the flux Richardson number and is a measure of dynamic stability.


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