Difference between revisions of "06/07/2014 16:00:00 UTC"
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=Comment Section= | =Comment Section= | ||
| + | *Very strong compressed magnetic field in the sheath region, in the possible cloud (the region with lower density and lower temperature) the magnetic field is pretty week. Given the high velocities before and after the low density region, there may be some CIR involvement. I think there is a CME here, but not a particularly strong flux rope. Given the weak magnetic field, possibly a flank passing event (Hess) | ||
=Image Data= | =Image Data= | ||
| + | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| + | [[File:plot_sw_mag_plasma_2014060700.png|350px]] | ||
| + | [[File:plot_sw_mag_2014060700.png|400px]] | ||
| + | [[File:plot_sw_vel_2014060700.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 13:52, 18 May 2015
Comment Section
- Very strong compressed magnetic field in the sheath region, in the possible cloud (the region with lower density and lower temperature) the magnetic field is pretty week. Given the high velocities before and after the low density region, there may be some CIR involvement. I think there is a CME here, but not a particularly strong flux rope. Given the weak magnetic field, possibly a flank passing event (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.
