Difference between revisions of "01/07/2015 05:47:08 UTC"
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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= | =Image Data= | ||
==In-Situ Data== | ==In-Situ Data== | ||
| − | A combination of | + | A combination of MFI and SWE data from the Wind Satellite: <br /> |
| − | + | ||
| − | [[File: | + | [[File:20150107_074917_20150107_202125.png|400px]] |
| − | + | ||
| − | The | + | The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock. |
| − | + | ||
=Video Data= | =Video Data= | ||
=References= | =References= | ||
Latest revision as of 11:14, 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:
Error creating thumbnail: File missing
The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.
