Difference between revisions of "02/19/2014 03:00:00 UTC"
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| + | 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= | ||
==In-Situ Data== | ==In-Situ Data== | ||
A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| − | [[File: | + | [[File:plot_sw_mag_plasma_2014021800_2.png|350px]] |
[[File:plot_sw_mag_2014021800.png|400px]] | [[File:plot_sw_mag_2014021800.png|400px]] | ||
[[File:plot_sw_vel_2014021800.png|350px]] <br /> | [[File:plot_sw_vel_2014021800.png|350px]] <br /> | ||
Latest revision as of 14:18, 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.
