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	<title>Approximate tangent space - Revision history</title>
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		<id>https://en.formulasearchengine.com/w/index.php?title=Approximate_tangent_space&amp;diff=30307&amp;oldid=prev</id>
		<title>en&gt;Michael Hardy at 01:27, 13 January 2014</title>
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		<updated>2014-01-13T01:27:08Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;In [[fluid dynamics]], the &amp;#039;&amp;#039;&amp;#039;Burgers vortex&amp;#039;&amp;#039;&amp;#039; is an exact solution to the [[Navier–Stokes equations]] governing [[viscous flow]]. The Burgers vortex describes a stationary, [[self-similarity|self-similar]] flow.&lt;br /&gt;
An inward, radial flow, tends to concentrate [[vorticity]] in a narrow column around the symmetry axis. On the same time, [[viscosity|viscous]] diffusion tends to spread the vorticity. The stationary Burgers vortex arises when the two effects balance.&lt;br /&gt;
&lt;br /&gt;
The Burgers vortex, apart from serving as an illustration of the [[vortex stretching]] mechanism, may describe such flows as tornados, where the vorticity is provided by continuous [[convection]]-driven vortex stretching.&lt;br /&gt;
&lt;br /&gt;
== Flow field ==&lt;br /&gt;
The flow for the Burgers vortex is described in cylindrical &amp;lt;math&amp;gt;(r,z,\phi)&amp;lt;/math&amp;gt; coordinates. Assuming axial symmetry (no &amp;lt;math&amp;gt;\phi&amp;lt;/math&amp;gt;-dependence), the [[vorticity equation]] is solved by the flow field:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;v_r=-\frac12 \alpha r,&amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;v_z=\alpha z,&amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;v_\phi=v_\phi(r),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\alpha&amp;gt;0&amp;lt;/math&amp;gt; is a constant. The flow satisfies the [[continuity equation]] by the two first of the above equations. The vorticity equation only gives a non-trivial component in the &amp;lt;math&amp;gt;z&amp;lt;/math&amp;gt;-direction, where it becomes&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{D\zeta}{D t}=\zeta\frac{\partial v_z}{\partial z}+\nu\nabla^2\zeta,&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;D/Dt&amp;lt;/math&amp;gt; denotes the [[convective derivative]] and &amp;lt;math&amp;gt;\nu&amp;lt;/math&amp;gt; the viscosity. Note that the first term on the right-hand side is the vortex stretching term which tends to &amp;#039;&amp;#039;amplify&amp;#039;&amp;#039; the vorticity, while he second term, due to viscosity, attenuates (or rather spreads) vorticity. The solution can be found as &lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\zeta=\zeta_0 \exp(-\frac{\alpha r^2}{4\nu}),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\zeta_0&amp;lt;/math&amp;gt; is a constant.&amp;lt;ref&amp;gt;{{cite book | last=Lautrup|first= Benny | title=Physics of Continuous Matter|edition= 2nd  | publisher=CRC Press | year=2011 | isbn=1420077007}}&amp;lt;/ref&amp;gt; The vorticity is thus distributed as a [[Gaussian function|Gaussian]] of width&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;R=2\sqrt{\frac{\nu}{\alpha}}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category:Fluid dynamics| ]]&lt;/div&gt;</summary>
		<author><name>en&gt;Michael Hardy</name></author>
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