<?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="Coronagraph - Page 7 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=coronagraph&amp;p=6">1.Previous</a><br />
<a accesskey="3" href="page.php?w=coronagraph&amp;p=8">3.Next</a>
</p>
<p>containing an opaque spot; this focal plane is reimaged onto a detector. Another arrangement is to image the sky onto a mirror with a small hole: the desired light is reflected and eventually reimaged, but the unwanted light from the star goes through the hole and does not reach the detector. Either way, the instrument design must take into account scattering and <a href="page.php?w=diffraction">diffraction</a> to make sure that as little unwanted light as possible reaches the final detector.  Lyot's key invention was an arrangement of lenses</p><p>
<a accesskey="1" href="page.php?w=coronagraph&amp;p=6">1.Previous</a><br />
<a accesskey="3" href="page.php?w=coronagraph&amp;p=8">3.Next</a>
</p>

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

</card>
</wml>
