Difference between revisions of "04/20/2014 11:00:00 UTC"
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| + | *Clear shock, followed by most of the standard MC signatures (low beta, low density, rotating magnetic field, etc.), but a fairly weak total magnetic field strength. The CME probably wasn't passing near the nose (Hess) | ||
=Image Data= | =Image Data= | ||
| + | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| + | [[File:plot_sw_mag_plasma_2014042000.png|350px]] | ||
| + | [[File:plot_sw_mag_2014042000.png|400px]] | ||
| + | [[File:plot_sw_vel_2014042000.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 14:02, 18 May 2015
Comment Section
- Clear shock, followed by most of the standard MC signatures (low beta, low density, rotating magnetic field, etc.), but a fairly weak total magnetic field strength. The CME probably wasn't passing near the nose (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.
