Latest revision as of 11:14, 18 September 2017

Comment Section

A typical shock and magnetic cloud. The velocity increased in the rear part of the magnetic cloud. There may be a CIR after this MC.(Yutian Chi).

A combination of MFI and SWE data from the Wind Satellite:

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The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.

@@ Line 1: / Line 1: @@
 =Comment Section=
-*At first glance this looks like a shock with a possible cloud after it, but the temperature and denisty peaks look more like a CIR. (Hess)
+*A typical shock and magnetic cloud. The velocity increased in the rear part of the magnetic cloud. There may be a CIR after this MC.(Yutian Chi).
 =Image Data=
 ==In-Situ Data==
-A combination of SWEPAM and MAG data from the Wind Satellite: <br />
+A combination of MFI and SWE data from the Wind Satellite: <br />
-[[File:plot_sw_mag_plasma_2014021401.png|350px]]
-[[File:plot_sw_mag_2014021400.png|400px]]
+[[File:20150107_074917_20150107_202125.png|400px]]
-[[File:plot_sw_vel_2014021400.png|350px]] <br />
-The blue lines are an approximation of the CME cloud and the red line denotes the shock.
+The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.
 =Video Data=
 =References=