Difference between revisions of "03/17/2013 05:30:00 UTC"
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[[File:plot_sw_vel_2013031600.png|350px]] <br /> | [[File:plot_sw_vel_2013031600.png|350px]] <br /> | ||
The blue lines are an approximation of the CME cloud and the red line denotes the shock. | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
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| + | ==Heliospheric Imager Data== | ||
| + | [[File:20120315stereoa.gif]] | ||
| + | [[File:20120315stereob.gif]] | ||
=Video Data= | =Video Data= | ||
=References= | =References= | ||
Revision as of 13:52, 19 June 2014
Contents
Comment Section
- This is a varSITI campaign event
- Depressed density and temperature as well as decreasing velocity are indicative of a flux rope, but with the weak magnetic field it may just be the flank passing through the Earth. Clear shock signatures in temperature and velocity and total B, more of a gradual increase in density. (Hess)
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
Heliospheric Imager Data
