http://solar.gmu.edu/heliophysics/index.php?action=history&feed=atom&title=02%2F13%2F2013_17%3A00%3A00_UTC02/13/2013 17:00:00 UTC - Revision history2026-05-31T01:17:12ZRevision history for this page on the wikiMediaWiki 1.31.0http://solar.gmu.edu/heliophysics/index.php?title=02/13/2013_17:00:00_UTC&diff=1922&oldid=prevPhess4: /* Comment Section */2013-07-03T20:35:26Z<p><span dir="auto"><span class="autocomment">Comment Section</span></span></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 20:35, 3 July 2013</td>
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<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>=Comment Section=</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>=Comment Section=</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>*It is difficult to see a lot in the heliospheric imagers corresponding to this event. My best guess is that, if there is a CME driver for this event, it is a plasma blob that can barely be seen in COR2A late on the 10th, and it takes more than a full day to accelerate out of the COR2 field of view. It was very faint and weak in LASCO. After taking more than a day to get out of COR2, it picks up enough speed to reach the Earth in less than 2 additional days. The blob may have been accelerated by another CME that occurred on the 12th. (Hess)</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>*It is difficult to see a lot in the heliospheric imagers corresponding to this event. My best guess is that, if there is a CME driver for this event, it is a plasma blob that can barely be seen in COR2A late on the 10th, and it takes more than a full day to accelerate out of the COR2 field of view. It was very faint and weak in LASCO <ins class="diffchange diffchange-inline">(The blob was so weak none of the SEEDS algorithms detected it in any instrument)</ins>. After taking more than a day to get out of COR2, it picks up enough speed to reach the Earth in less than 2 additional days. The blob may have been accelerated by another CME that occurred on the 12th. (Hess)</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>=Image Data=</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>=Image Data=</div></td></tr>
</table>Phess4http://solar.gmu.edu/heliophysics/index.php?title=02/13/2013_17:00:00_UTC&diff=1921&oldid=prevPhess4: /* Comment Section */2013-07-03T20:33:32Z<p><span dir="auto"><span class="autocomment">Comment Section</span></span></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 20:33, 3 July 2013</td>
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<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>=Comment Section=</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>=Comment Section=</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>*It is difficult to see a lot in the heliospheric imagers corresponding to this event. My best guess is that, if there is a CME driver for this event, it is a plasma blob that can barely be seen late on the 10th, and it takes more than a full day to accelerate out of the COR2 field of view. It was very faint and weak <del class="diffchange diffchange-inline">and barely seen by </del>LASCO. After <del class="diffchange diffchange-inline">not </del>taking more than a day to get out of COR2, it picks up enough speed to reach the Earth in less than 2 days. The blob may have been accelerated by another CME that occurred on the 12th. (Hess)</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>*It is difficult to see a lot in the heliospheric imagers corresponding to this event. My best guess is that, if there is a CME driver for this event, it is a plasma blob that can barely be seen <ins class="diffchange diffchange-inline">in COR2A </ins>late on the 10th, and it takes more than a full day to accelerate out of the COR2 field of view. It was very faint and weak <ins class="diffchange diffchange-inline">in </ins>LASCO. After taking more than a day to get out of COR2, it picks up enough speed to reach the Earth in less than 2 <ins class="diffchange diffchange-inline">additional </ins>days. The blob may have been accelerated by another CME that occurred on the 12th. (Hess)</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>=Image Data=</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>=Image Data=</div></td></tr>
</table>Phess4http://solar.gmu.edu/heliophysics/index.php?title=02/13/2013_17:00:00_UTC&diff=1920&oldid=prevPhess4: /* Comment Section */2013-07-03T20:32:53Z<p><span dir="auto"><span class="autocomment">Comment Section</span></span></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 20:32, 3 July 2013</td>
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<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>=Comment Section=</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>=Comment Section=</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><ins class="diffchange diffchange-inline">*It is difficult to see a lot in the heliospheric imagers corresponding to this event. My best guess is that, if there is a CME driver for this event, it is a plasma blob that can barely be seen late on the 10th, and it takes more than a full day to accelerate out of the COR2 field of view. It was very faint and weak and barely seen by LASCO. After not taking more than a day to get out of COR2, it picks up enough speed to reach the Earth in less than 2 days. The blob may have been accelerated by another CME that occurred on the 12th. (Hess)</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>=Image Data=</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>=Image Data=</div></td></tr>
</table>Phess4http://solar.gmu.edu/heliophysics/index.php?title=02/13/2013_17:00:00_UTC&diff=1736&oldid=prevPhess4: /* In-Situ Data */2013-07-01T20:48:42Z<p><span dir="auto"><span class="autocomment">In-Situ Data</span></span></p>
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<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>A combination of SWEPAM and MAG data from the ACE Satellite: <br /></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>A combination of SWEPAM and MAG data from the ACE Satellite: <br /></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">[[File:plot_sw_mag_2013021300.png|400px]]</ins></div></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 class="diffchange diffchange-inline">[[File:plot_sw_vel_2013021300.png|350px]] <br /></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;"><div>The blue lines are an approximation of the CME cloud and the red line denotes the shock.</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>The blue lines are an approximation of the CME cloud and the red line denotes the shock.</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>
</table>Phess4http://solar.gmu.edu/heliophysics/index.php?title=02/13/2013_17:00:00_UTC&diff=1683&oldid=prevPhess4: Created page with "=Comment Section= =Image Data= ==In-Situ Data== A combination of SWEPAM and MAG data from the ACE Satellite: <br /> The blue lines are an approximation of the CME cloud and..."2013-07-01T16:25:57Z<p>Created page with "=Comment Section= =Image Data= ==In-Situ Data== A combination of SWEPAM and MAG data from the ACE Satellite: <br /> The blue lines are an approximation of the CME cloud and..."</p>
<p><b>New page</b></p><div>=Comment Section=<br />
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=Image Data=<br />
==In-Situ Data==<br />
A combination of SWEPAM and MAG data from the ACE Satellite: <br /><br />
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.<br />
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=Video Data=<br />
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=References=</div>Phess4