http://naturalphilosophy.org/wiki/index.php?action=history&feed=atom&title=The_Spectrum_of_the_Universe 2026-04-09T21:58:43Z Revision history for this page on the wiki MediaWiki 1.43.0 http://naturalphilosophy.org/wiki/index.php?title=The_Spectrum_of_the_Universe&diff=21818&oldid=prev 2017-01-01T18:27:14Z

<p>Imported from text file</p> <table style="background-color: #fff; color: #202122;" data-mw="interface"> <col class="diff-marker" /> <col class="diff-content" /> <col class="diff-marker" /> <col class="diff-content" /> <tr class="diff-title" lang="en"> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">← Older revision</td> <td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 14:27, 1 January 2017</td> </tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l14">Line 14:</td> <td colspan="2" class="diff-lineno">Line 14:</td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>The Universe has several maxima of radiation. The largest maximum, which is called the ?relic mximum?, arises from the process of hydrogen atom fusion at the start of the Universe. The smallest maxima, being called the infrared radiation sources, are formed by the processes of hydrogen molecule fusion in the vicinity of the stars, and their liquefaction in the Universe.</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>The Universe has several maxima of radiation. The largest maximum, which is called the ?relic mximum?, arises from the process of hydrogen atom fusion at the start of the Universe. The smallest maxima, being called the infrared radiation sources, are formed by the processes of hydrogen molecule fusion in the vicinity of the stars, and their liquefaction in the Universe.</div></td></tr> <tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><br></td></tr> <tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>&lt;/span&gt;[[Category:Scientific Paper]]</div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>&lt;/span&gt;</div></td></tr> <tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div> </div></td></tr> <tr><td colspan="2" class="diff-side-deleted"></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>[[Category:Scientific Paper<ins style="font-weight: bold; text-decoration: none;">|spectrum universe</ins>]]</div></td></tr> </table>

Maintenance script http://naturalphilosophy.org/wiki/index.php?title=The_Spectrum_of_the_Universe&diff=3546&oldid=prev 2016-12-30T05:17:33Z

<p>Imported from text file</p> <p><b>New page</b></p><div>{{Infobox paper<br /> | title = The Spectrum of the Universe<br /> | author = [[Philipp M Kanarev]]<br /> | keywords = [[photon]], [[electron]], [[spectrum]], [[hydrogen atom]], [[hydrogen molecule]], [[temperature]], [[wavelength]]<br /> | published = 2009<br /> | journal = [[Galilean Electrodynamics]]<br /> | volume = [[20]]<br /> | number = [[S1]]<br /> | pages = 13-17<br /> }}<br /> <br /> ==Abstract==<br /> <br /> The Universe has several maxima of radiation. The largest maximum, which is called the ?relic mximum?, arises from the process of hydrogen atom fusion at the start of the Universe. The smallest maxima, being called the infrared radiation sources, are formed by the processes of hydrogen molecule fusion in the vicinity of the stars, and their liquefaction in the Universe.<br /> <br /> &lt;/span&gt;[[Category:Scientific Paper]]</div>

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