Difference between revisions of "List of CMEs for WG5 Analysis"
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| 2010-04-03T09:54 UT | | 2010-04-03T09:54 UT | ||
| AR NOAA 11059 | | AR NOAA 11059 | ||
| − | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/8675/1 | + | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [[https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/8675/1 CCMC donki details]] |
|Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [[http://dx.doi.org/10.1002/2015SW001171 10.1002/2015SW001171]] | |Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [[http://dx.doi.org/10.1002/2015SW001171 10.1002/2015SW001171]] | ||
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| 2011-08-02T06:40 UT | | 2011-08-02T06:40 UT | ||
| AR NOAA 11261 | | AR NOAA 11261 | ||
| − | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/25/1 | + | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [[https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/25/1 CCMC donki details]] |
|Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions | |Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions | ||
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| 2012-07-12T16:54 UT | | 2012-07-12T16:54 UT | ||
| AR NOAA 11520 | | AR NOAA 11520 | ||
| − | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/14/1 | + | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [[https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/14/1 CCMC donki details]] |
|Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [[http://dx.doi.org/10.1002/2015SW001171 10.1002/2015SW001171]] | |Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [[http://dx.doi.org/10.1002/2015SW001171 10.1002/2015SW001171]] | ||
| Line 63: | Line 63: | ||
|2013-07-09T15:09 UT | |2013-07-09T15:09 UT | ||
| N20E15 prominence | | N20E15 prominence | ||
| − | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/32/2 | + | | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [[https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/32/2 CCMC donki details]] |
|Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions | |Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions | ||
| | | | ||
| N. Savani (neel.savani@nasa.gov)} | | N. Savani (neel.savani@nasa.gov)} | ||
Latest revision as of 17:09, 18 July 2018
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)} | |
| 2012/03/07 01:14 UT | AR NOAA 11429 | The coronal CME magnetic field is estimated by combination of magnetic helicity calculations of the CME source region and forward modeling of the CME along with application of the helicity conservation principle in flux-rope CMEs | Patsourakos, S., Georgoulis, M. K., Vourlidas, A. et al., 2016, ApJ, 817, 14 | S. Patsourakos (spatsour@cc.uoi.gr)} | |
| 2010-04-03T09:54 UT | AR NOAA 11059 | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [CCMC donki details] | Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [10.1002/2015SW001171]
Savani, N. P., Vourlidas, A. et al., 2017, Space Weather, 15: 441 [10.1002/2016SW001458] Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions |
N. Savani (neel.savani@nasa.gov)} | |
| 2011-08-02T06:40 UT | AR NOAA 11261 | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [CCMC donki details] | Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions | N. Savani (neel.savani@nasa.gov)} | |
| 2012-07-12T16:54 UT | AR NOAA 11520 | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [CCMC donki details] | Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [10.1002/2015SW001171]
Savani, N. P., Vourlidas, A. et al., 2017, Space Weather, 15: 441 [10.1002/2016SW001458] Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions |
N. Savani (neel.savani@nasa.gov)} | |
| 2013-07-09T15:09 UT | N20E15 prominence | Bz prediction and Kp prediction was using the Bz4Cast model. To be used by IMF Bz team as core event list for MHD modelers. [CCMC donki details] | Savani, N. P., et al., 2018, Space Weather, special issue, Skill metric evaluation by a Community International Forum for Interplanetary Magnetic Field Bz predictions | N. Savani (neel.savani@nasa.gov)} |
