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| − | *A typical shock and magnetic cloud(Yutian Chi). | + | *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= | =Image Data= | ||
Revision as of 12:05, 18 September 2017
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:
The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.
