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| + | *Definite shock, rotation in mangetic field and weak signatures in velocity, density and temperature indicate there is likely a weak flux rope behind the shock. (Hess) | ||
=Image Data= | =Image Data= | ||
Revision as of 12:41, 29 August 2014
Comment Section
- Definite shock, rotation in mangetic field and weak signatures in velocity, density and temperature indicate there is likely a weak flux rope behind the shock. (Hess)
Image Data
In-Situ 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.
