View source for 03/17/2013 05:30:00 UTC

=Comment Section=
*This is a varSITI campaign event for ISEST and SPeCIMEN. 

At the Sun the event had an M1.1 flare, erupting filament, type IV radio burst, fast halo CME. At Earth a shock, possible MC, SEP, and strong storm, Dst=-132. A TB case. Modeled by C-C Wu. 

*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: <br />
[[File:plot_sw_mag_plasma_2013031600.png|350px]]
[[File:plot_sw_mag_2013031600.png|400px]]
[[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.

==Heliospheric Imager Data==
[[File:20120315stereoa.gif]]
[[File:20120315stereob.gif]]

=Video Data=
[http://solar.gmu.edu/wiki/upload/phess4/20120315aia171.mp4 AIA 171] <br>
[http://solar.gmu.edu/wiki/upload/phess4/20120315aia193.mp4 AIA 193] <br>
[http://solar.gmu.edu/wiki/upload/phess4/20120315hmi.mp4 HMI] <br>

=References=