Difference between revisions of "List of CMEs for WG5 Analysis"
| Line 13: | Line 13: | ||
| 2011/06/07 06:47 UT | | 2011/06/07 06:47 UT | ||
| AR NOAA 11226 (CME propagating on the west limb) | | AR NOAA 11226 (CME propagating on the west limb) | ||
| − | | The magnetic field | + | | The magnetic field 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 |
| − | | | + | | Bemporad, A. & Mancuso, S. 2010, ApJ 720, 130 (also Bemporad, A., Susino, R., & Mancso, S. ApJ, in preparation) |
| | | | ||
| R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)} | | R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)} | ||
Revision as of 11:47, 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 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 | Bemporad, A. & Mancuso, S. 2010, ApJ 720, 130 (also Bemporad, A., Susino, R., & Mancso, S. ApJ, in preparation) | R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)} |
