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      <p ns="0" title="Incompressible flow" snippet="...city, the magnitude of velocity gradient is &amp;lt;math&amp;gt;U/L&amp;lt;/math&amp;gt;. The physical &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; of the incompressible flow is &#10;" size="8372" wordcount="1427" timestamp="2013-08-19T18:57:10Z" />
      <p ns="0" title="Gauss-Seidel method" snippet="...ible diagonal dominance of the system is sufficient to ensure convergence, &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; the method will work.&#10;" size="8589" wordcount="1113" timestamp="2012-01-03T09:15:07Z" />
      <p ns="0" title="Combustion" snippet="...(see [[#Damk&amp;amp;ouml;hler Number|Sec. Damk&amp;amp;ouml;hler Number]] for the general &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; of the Damk&amp;amp;ouml;hler):&#10;...&amp;amp;ouml;hler number is expected to be around unity in the extinction regime, &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; that the &#039;&#039;Da&#039;&#039; is still high enough to sustain combustion but that the non&#10;" size="159468" wordcount="25897" timestamp="2011-03-17T22:14:20Z" />
      <p ns="0" title="Solution of Navier-Stokes equations" snippet="... for both turbulent or laminar flows, with some modification of the actual &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; of individual terms.&#10;" size="2184" wordcount="330" timestamp="2009-04-23T10:01:48Z" />
      <p ns="0" title="Continuum" snippet="...terms velocity, acceleration, density and pressure etc. at a point have no &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt;. For instance, density is equal to zero at point, if that point does not co&#10;" size="1073" wordcount="180" timestamp="2005-11-22T21:40:31Z" />
      <p ns="0" title="Introduction to turbulence/Statistical analysis/Ensemble average" snippet="...s a single time. The key is that they must all be &#039;&#039;independent events&#039;&#039; - &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; the probability of achieving a head or tail in a given flip must be complet&#10;" size="8372" wordcount="1391" timestamp="2011-07-02T12:29:56Z" />
      <p ns="0" title="Introduction to turbulence/Turbulence kinetic energy" snippet="...sure. Only the integral scale, &amp;lt;math&amp;gt;L&amp;lt;/math&amp;gt;, is a physical length scale, &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; that it can be directly observed in the flow by spectral or correlation mea&#10;" size="48000" wordcount="7664" timestamp="2013-12-13T12:47:53Z" />
      <p ns="0" title="Introduction to turbulence/Free turbulent shear flows" snippet="... have been waged over less), then you better be dealing with a full desk - &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; these second order terms had better be retained in any calculation or exper&#10;... almost always does. Such a search is called the search for &amp;quot;&#039;&#039;scales&#039;&#039;&amp;quot; , &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; &amp;quot;&#039;&#039;scales&#039;&#039;&amp;quot; which collapse the data. Now precisely what does &amp;quot;collapse the&#10;" size="68433" wordcount="11204" timestamp="2016-04-19T13:42:18Z" />
      <p ns="0" title="Heaviside function" snippet="...n make sense) for &#039;&#039;x&#039;&#039; = 0, depending on which formalism one uses to give &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; to integrals involving &#039;&#039;δ&#039;&#039;.&#10;" size="1360" wordcount="200" timestamp="2008-07-13T23:11:04Z" />
      <p ns="0" title="Introduction to turbulence/Wall bounded turbulent flows" snippet="unity; i.e. &amp;lt;math&amp;gt; u_{*} \eta / \nu = 1 &amp;lt;/math&amp;gt;, &lt;span class=&#039;searchmatch&#039;&gt;meaning&lt;/span&gt; that viscous and inertial terms are about the same. But then this is precis&#10;" size="42418" wordcount="7002" timestamp="2012-03-21T13:02:46Z" />
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