<?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="Cosmic background radiation - Page 6 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=cosmic_background_radiation&amp;p=5">1.Previous</a><br />
<a accesskey="3" href="page.php?w=cosmic_background_radiation&amp;p=7">3.Next</a>
</p>
<p>of 3.2&nbsp;K. </p>

<p>1930s:<a href="page.php?w=Erich_Regener">Erich Regener</a> calculates that the non-thermal spectrum of cosmic rays in the galaxy has an effective temperature of 2.8&nbsp;K.</p>

<p>1931:The term microwave first appears in print: "When trials with wavelengths as low as 18&nbsp;cm were made known, there was undisguised surprise that the problem of the micro-wave had been solved so soon." Telegraph & Telephone Journal XVII. 179/1"</p>

<p>1938:<a href="page.php?w=Walther_Nernst">Walther Nernst</a> re-estimates the cosmic</p><p>
<a accesskey="1" href="page.php?w=cosmic_background_radiation&amp;p=5">1.Previous</a><br />
<a accesskey="3" href="page.php?w=cosmic_background_radiation&amp;p=7">3.Next</a>
</p>

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

</card>
</wml>
