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

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(Comment Section)
(Image Data)
 
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=Comment Section=
 
=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. <br>
 
*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. <br>
*At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown.  
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*At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. (Yutian)
(Yutian)
 
  
 
=Image Data=
 
=Image Data=
 
A combination of MFI and SWE data from the Wind Satellite: <br />
 
A combination of MFI and SWE data from the Wind Satellite: <br />
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[[File:Example.jpg|400px]]
  
 
The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.
 
The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.

Latest revision as of 12:14, 18 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.
  • At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. (Yutian)

Image Data

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

Error creating thumbnail: File missing

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

Video Data

References