Difference between revisions of "03/31/2015 07:31:49 UTC"
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=Comment Section= | =Comment Section= | ||
*Clear shock, followed by most of the standard MC signatures (low beta, low density, smooth magnetic field, etc.), but a fairly weak magnetic field rotation. <br> | *Clear shock, followed by most of the standard MC signatures (low beta, low density, smooth magnetic field, etc.), but a fairly weak magnetic field rotation. <br> | ||
| − | *At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. | + | *At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. (Yutian) |
| − | (Yutian) | ||
=Image Data= | =Image Data= | ||
Revision as of 13:28, 16 September 2017
Comment Section
- Clear shock, followed by most of the standard MC signatures (low beta, low density, smooth magnetic field, etc.), but a fairly weak magnetic field rotation.
- At 03/27/2015 15:12:08, there may be a partial halo CME corresponding to this magnetic cloud. The solar source of this CME is unknown. (Yutian)
Image Data
A combination of MFI and SWE data from the Wind Satellite:
The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock.
