03/31/2015 07:31:49 UTC

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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)

[[File:]]=Image Data= A combination of MFI and SWE data from the Wind Satellite:

Example.jpg

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

Video Data

References

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