Difference between revisions of "List of CMEs for WG5 Analysis"
| Line 11: | Line 11: | ||
|- USER ENTRY ADD your inputs in blocks such as the following | |- USER ENTRY ADD your inputs in blocks such as the following | ||
| − | | | + | | 2011/06/07 06:47 UT |
| − | | | + | | AR NOAA 11226 (CME propagating on the west limb) |
| − | | | + | | The magnetic field strength in the corona is determined by applying the Rankine-Hugoniot equations to LASCO C2 and C3 white-light images of the CME-driven shock in order to derive a map of the shock Alfvenic Mach number |
| − | | | + | | http://adsabs.harvard.edu/abs/2014cosp...40E.272B (ApJ in preparation) |
| − | | | + | | |
| − | | | + | | R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)} |
| − | |||
Revision as of 10:32, 10 March 2015
List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5
| Date and Time | Solar Source (AR # or location) | Method of Magnetic Field Determination | Publication | Miscellaneous | Submitter contact |
|---|---|---|---|---|---|
| 2011/06/07 06:47 UT | AR NOAA 11226 (CME propagating on the west limb) | The magnetic field strength in the corona is determined by applying the Rankine-Hugoniot equations to LASCO C2 and C3 white-light images of the CME-driven shock in order to derive a map of the shock Alfvenic Mach number | http://adsabs.harvard.edu/abs/2014cosp...40E.272B (ApJ in preparation) | R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)} |
