01/07/2015 05:47:08 UTC

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Revision as of 11:14, 18 September 2017 by Ytchi (talk | contribs) (In-Situ Data)
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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).

Image Data

In-Situ Data

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.

Video Data

References