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	<title>09/07/2017 23:30:00 UTC - Revision history</title>
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	<updated>2026-06-01T07:03:02Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>http://solar.gmu.edu/heliophysics/index.php?title=09/07/2017_23:30:00_UTC&amp;diff=2949&amp;oldid=prev</id>
		<title>Phess4: Created page with &quot;=Comment Section= *Strong C2 halo with a flux rope oriented towards the southwest erupting around 12:00 UT on the 6th leads to a strong shock with a pretty clear magnetic clou...&quot;</title>
		<link rel="alternate" type="text/html" href="http://solar.gmu.edu/heliophysics/index.php?title=09/07/2017_23:30:00_UTC&amp;diff=2949&amp;oldid=prev"/>
		<updated>2018-08-08T15:58:20Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;=Comment Section= *Strong C2 halo with a flux rope oriented towards the southwest erupting around 12:00 UT on the 6th leads to a strong shock with a pretty clear magnetic clou...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;=Comment Section=&lt;br /&gt;
*Strong C2 halo with a flux rope oriented towards the southwest erupting around 12:00 UT on the 6th leads to a strong shock with a pretty clear magnetic cloud. From the inferred transit time of about 36 hours, this is clearly a very fast CME. The source is the same active region that spawned the much studied limb X flare and fast CME a few days later on the 10th. (Hess)&lt;br /&gt;
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=Image Data=&lt;br /&gt;
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=Video Data=&lt;br /&gt;
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=References=&lt;/div&gt;</summary>
		<author><name>Phess4</name></author>
		
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