Difference between revisions of "03/31/2015 07:31:49 UTC"

From heliophysics
Jump to: navigation, search
(Comment Section)
(Image Data)
Line 3: Line 3:
  
 
=Image Data=
 
=Image Data=
A combination of SWEPAM and MAG data from the ACE Satellite: <br />
+
A combination of MFI and SWE data from the Wind Satellite: <br />
[[File:plot_sw_mag_plasma_2014042000.png|350px]]
+
 
[[File:plot_sw_mag_2014042000.png|400px]]
+
The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.
[[File:plot_sw_vel_2014042000.png|350px]] <br />
 
The blue lines are an approximation of the CME cloud and the red line denotes the shock.
 
  
 
=Video Data=
 
=Video Data=
  
 
=References=
 
=References=

Revision as of 13:09, 16 September 2017

Comment Section

  • Clear shock, followed by most of the standard MC signatures (low beta, low density, smooth magnetic field, etc.), but a fairly weak magnetic field rotation. (Yutian)

Image Data

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

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

Video Data

References