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<a accesskey="3" href="page.php?w=Solar_prominence&amp;p=2">3.Next</a>
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<p>In <a href="page.php?w=solar_physics">solar physics</a>, a <b>prominence</b>, sometimes referred to as a <b>filament</b>, is a large <a href="page.php?w=Plasma_%28physics%29">plasma</a> and <a href="page.php?w=magnetic_field">magnetic field</a> structure extending outward from the <a href="page.php?w=Sun">Sun</a>'s surface, often in a loop shape. Prominences are anchored to the Sun's surface in the much brighter <a href="page.php?w=photosphere">photosphere</a>, and extend outwards into the <a href="page.php?w=solar_corona">solar corona</a>. </p><p>
<a accesskey="3" href="page.php?w=Solar_prominence&amp;p=2">3.Next</a>
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