Difference between revisions of "03/25/2014 19:30:00 UTC"
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| + | *Definite shock, rotation in mangetic field and weak signatures in velocity, density and temperature indicate there is may be a weak flux rope behind the shock. There are a number of eruptions between the 20-22, but none are full Halo CMEs. The most patial Halo is on the 20th. It is also possible that this event is a combination of multiple eruptions. (Hess) | ||
=Image Data= | =Image Data= | ||
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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:plot_sw_mag_plasma_2014032500.png|350px]] | [[File:plot_sw_mag_plasma_2014032500.png|350px]] | ||
| − | [[File: | + | [[File:plot_sw_mag_2014032500_2.png|400px]] |
[[File:plot_sw_vel_2014032500.png|350px]] <br /> | [[File:plot_sw_vel_2014032500.png|350px]] <br /> | ||
The blue lines are an approximation of the CME cloud and the red line denotes the shock. | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
Latest revision as of 13:25, 29 August 2014
Comment Section
- Definite shock, rotation in mangetic field and weak signatures in velocity, density and temperature indicate there is may be a weak flux rope behind the shock. There are a number of eruptions between the 20-22, but none are full Halo CMEs. The most patial Halo is on the 20th. It is also possible that this event is a combination of multiple eruptions. (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.
