Difference between revisions of "02/19/2014 03:00:00 UTC"
(→Comment Section) |
(→Comment Section) |
||
| Line 1: | Line 1: | ||
=Comment Section= | =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) | + | 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. one of which is likely the Halo CME on Feb. 16. (Hess) |
=Image Data= | =Image Data= | ||
Latest revision as of 13:18, 29 August 2014
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. one of which is likely the Halo CME on Feb. 16. (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.
