Difference between revisions of "04/05/2014 10:00:00 UTC"
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=Comment Section= | =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= | =Image Data= | ||
| + | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| + | [[File:plot_sw_mag_plasma_2014040500.png|350px]] | ||
| + | [[File:plot_sw_mag_2014040500.png|400px]] | ||
| + | [[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. | ||
=Video Data= | =Video Data= | ||
=References= | =References= | ||
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:
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Error creating thumbnail: File missing
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
