02/19/2014 03:00:00 UTC

From heliophysics
Revision as of 12:37, 29 August 2014 by Phess4 (talk | contribs) (Comment Section)
Jump to: navigation, search

Comment Section

Obvious shock jumps in B and V, but density shows only a later, gradual increase. There is a possible small magnetic cloud after the shock, as well as a weak cloud directly infront of it. This is likely an interaction of multiple events. (Hess)

Image Data

In-Situ Data

A combination of SWEPAM and MAG data from the ACE Satellite:

Error creating thumbnail: File missing
Error creating thumbnail: File missing
Error creating thumbnail: File missing


The blue lines are an approximation of the CME cloud and the red line denotes the shock.

Video Data

References