http://icrpaedia.org/index.php?title=Low_Earth_orbit&feed=atom&action=historyLow Earth orbit - Revision history2024-03-28T18:57:23ZRevision history for this page on the wikiMediaWiki 1.32.0http://icrpaedia.org/index.php?title=Low_Earth_orbit&diff=3290&oldid=prevChris Clement at 01:58, 20 August 20212021-08-20T01:58:40Z<p></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 01:58, 20 August 2021</td>
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<tr><td class='diff-marker'>−</td><td style="color: #222; 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>Orbit in space near to the Earth where astronauts are protected against parts of particles of galactic and solar origin by the Earth’s magnetic field. The shielding depends on the inclination of the spacecraft. On the other hand, the Earth’s magnetic field is responsible for formation of the trapped radiation belts where (mainly) protons and electrons from galactic and solar origin are stored. <del class="diffchange diffchange-inline">([[ICRP Publication 123]], 2013)</del></div></td><td class='diff-marker'>+</td><td style="color: #222; 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><ins class="diffchange diffchange-inline">[[File:Glossary Icon-2.png|100px|frameless|right|link=ICRP Glossary]]</ins></div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; 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> </div></td><td class='diff-marker'>+</td><td style="color: #222; 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>Orbit in space near to the Earth where astronauts are protected against parts of particles of galactic and solar origin by the Earth’s magnetic field. The shielding depends on the inclination of the spacecraft. On the other hand, the Earth’s magnetic field is responsible for formation of the trapped radiation belts where (mainly) protons and electrons from galactic and solar origin are stored.</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; 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><del class="diffchange diffchange-inline">''ICRP Glossary entry - May 2019''</del></div></td><td colspan="2"> </td></tr>
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<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="color: #222; 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><ins style="font-weight: bold; text-decoration: none;">[[ICRP Publication 123]], 2013</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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>'''Return to [[ICRP Glossary|Glossary]]'''</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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>'''Return to [[ICRP Glossary|Glossary]]'''</div></td></tr>
</table>Chris Clementhttp://icrpaedia.org/index.php?title=Low_Earth_orbit&diff=2191&oldid=prevKaren Clement at 13:03, 13 September 20192019-09-13T13:03:44Z<p></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 13:03, 13 September 2019</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l1" >Line 1:</td>
<td colspan="2" class="diff-lineno">Line 1:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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>Orbit in space near to the Earth where astronauts are protected against parts of particles of galactic and solar origin by the Earth’s magnetic field. The shielding depends on the inclination of the spacecraft. On the other hand, the Earth’s magnetic field is responsible for formation of the trapped radiation belts where (mainly) protons and electrons from galactic and solar origin are stored. ([[ICRP Publication 123]], 2013)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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>Orbit in space near to the Earth where astronauts are protected against parts of particles of galactic and solar origin by the Earth’s magnetic field. The shielding depends on the inclination of the spacecraft. On the other hand, the Earth’s magnetic field is responsible for formation of the trapped radiation belts where (mainly) protons and electrons from galactic and solar origin are stored. ([[ICRP Publication 123]], 2013)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; 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;"></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="color: #222; 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><ins style="font-weight: bold; text-decoration: none;">''ICRP Glossary entry - May 2019''</ins></div></td></tr>
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<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="color: #222; 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>''<ins class="diffchange diffchange-inline">'Return to </ins>[[ICRP <ins class="diffchange diffchange-inline">Glossary|</ins>Glossary]]<ins class="diffchange diffchange-inline">'</ins>''</div></td></tr>
</table>Karen Clementhttp://icrpaedia.org/index.php?title=Low_Earth_orbit&diff=1445&oldid=prevIntern: Created page with "Orbit in space near to the Earth where astronauts are protected against parts of particles of galactic and solar origin by the Earth’s magnetic field. The shielding depends..."2019-06-10T15:22:29Z<p>Created page with "Orbit in space near to the Earth where astronauts are protected against parts of particles of galactic and solar origin by the Earth’s magnetic field. The shielding depends..."</p>
<p><b>New page</b></p><div>Orbit in space near to the Earth where astronauts are protected against parts of particles of galactic and solar origin by the Earth’s magnetic field. The shielding depends on the inclination of the spacecraft. On the other hand, the Earth’s magnetic field is responsible for formation of the trapped radiation belts where (mainly) protons and electrons from galactic and solar origin are stored. ([[ICRP Publication 123]], 2013)<br />
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''[[ICRP Glossary]] entry - May 2019''</div>Intern