<?xml version="1.0" encoding='utf-8'?>
<!DOCTYPE wml PUBLIC "-//WAPFORUM//DTD WML 1.1//EN" "http://www.wapforum.org/DTD/wml_1.1.xml">
<wml>
<card id="card1" title="Convection - Page 22 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=Convection&amp;p=21">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Convection&amp;p=23">3.Next</a>
</p>
<p>ice. It has also been proposed for <a href="page.php?w=Europa_%28moon%29">Europa</a>, and other bodies in the outer Solar System.</p>

<p><big> Thermomagnetic convection </big></p>
<p><b>Thermomagnetic convection</b> can occur when an external magnetic field is imposed on a <a href="page.php?w=ferrofluid">ferrofluid</a> with varying <a href="page.php?w=magnetic_susceptibility">magnetic susceptibility</a>. In the presence of a temperature gradient this results in a nonuniform magnetic body force, which leads to fluid movement. A ferrofluid is a liquid</p><p>
<a accesskey="1" href="page.php?w=Convection&amp;p=21">1.Previous</a><br />
<a accesskey="3" href="page.php?w=Convection&amp;p=23">3.Next</a>
</p>

<do type="prev" label="Search">
        <go href="search.wml"/>
</do>

</card>
</wml>
