Difference between revisions of "03/31/2015 07:31:49 UTC"
(→Comment Section) |
(→Image Data) |
||
| Line 3: | Line 3: | ||
*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) | *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= | + | [[File:]]=Image Data= |
A combination of MFI and SWE data from the Wind Satellite: <br /> | A combination of MFI and SWE data from the Wind Satellite: <br /> | ||
| + | |||
| + | [[File:Example.jpg]] | ||
The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock. | The grey region shows an approximation of the CME cloud and the red vertical line denotes the shock. | ||
Revision as of 10:46, 18 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)
[[File:]]=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.
