Difference between revisions of "02/19/2014 03:00:00 UTC"

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(Created page with "=Comment Section= =Image Data= ==In-Situ Data== A combination of SWEPAM and MAG data from the ACE Satellite: <br /> 350px [[File:pl...")
 
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=Comment Section=
 
=Comment Section=
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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:plot_sw_mag_plasma_2014021800.png|350px]]
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[[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 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.

Video Data

References