Difference between revisions of "03/31/2015 07:31:49 UTC"
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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 | + | *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) |
=Image Data= | =Image Data= | ||
Revision as of 13:04, 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. (Yutian)
Image Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
