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<a accesskey="3" href="page.php?w=Fraunhofer_lines&amp;p=2">3.Next</a>
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<p><a href="page.php?w=Image%3ASpectrum_of_blue_sky.svg">thumb</a>The <b>Fraunhofer lines</b> are a set of <a href="page.php?w=spectral_line">spectral absorption lines</a>. They are dark <a href="page.php?w=absorption_line">absorption line</a>s, seen in the <a href="page.php?w=optical_spectrum">optical spectrum</a> of the <a href="page.php?w=Sun">Sun</a>, and are formed when atoms in the <a href="page.php?w=solar_atmosphere">solar atmosphere</a> absorb light being emitted by the <a href="page.php?w=solar_photosphere">solar photosphere</a>. The lines</p><p>
<a accesskey="3" href="page.php?w=Fraunhofer_lines&amp;p=2">3.Next</a>
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