Difference between revisions of "04/05/2014 10:00:00 UTC"

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(Image Data)
(Comment Section)
 
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=Comment Section=
 
=Comment Section=
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*The compression wave in front of the possible cloud is probably to weak to be a shock though there are some shock like signatures. Strong magnetic field enhancement, but almost all of it is in the x and y directions with very little Bz at all. This may have been a highly tilted CME or one that passed close to the top or bottom of the flux rope. (Hess)
  
 
=Image Data=
 
=Image 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_2014040500.png|350px]]
 
[[File:plot_sw_mag_plasma_2014040500.png|350px]]
[[File:plot_sw_mag_2014040500_2.png|400px]]
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[[File:plot_sw_mag_2014040500.png|400px]]
 
[[File:plot_sw_vel_2014040500.png|350px]] <br />
 
[[File:plot_sw_vel_2014040500.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 14:07, 18 May 2015

Comment Section

  • The compression wave in front of the possible cloud is probably to weak to be a shock though there are some shock like signatures. Strong magnetic field enhancement, but almost all of it is in the x and y directions with very little Bz at all. This may have been a highly tilted CME or one that passed close to the top or bottom of the flux rope. (Hess)

Image 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