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

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(Image Data)
(Comment Section)
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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. (Yutian)
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*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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(Yutian)
  
 
=Image Data=
 
=Image Data=

Revision as of 14:27, 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.
  • 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:

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

Video Data

References