Difference between revisions of "List of CMEs for WG5 Analysis"

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(New IMF Bz team core event)
(added core event list implemented by MHD modelers for metric prototyping)
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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. It is also in the IMF Bz team core event list for MHD modelers. [https://kauai.ccmc.gsfc.nasa.gov/DONKI/view/CME/8675/1][[CCMC donki details]]
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| 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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Savani, N. P., Vourlidas, A. et al., 2017, Space Weather, 15: 441 [http://dx.doi.org/10.1002/2016SW001458][[10.1002/2016SW001458]]
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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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|
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| N. Savani (neel.savani@nasa.gov)}
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 +
|- USER ENTRY ADD your inputs in blocks such as the following
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| 2011-08-02T06:40 UT
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| AR NOAA 11261
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| 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]]
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|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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|
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| N. Savani (neel.savani@nasa.gov)}
 +
 +
|- USER ENTRY ADD your inputs in blocks such as the following
 +
| 2012-07-12T16:54 UT
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| AR NOAA 11520
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| 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., 2017, Space Weather, 15: 441 [http://dx.doi.org/10.1002/2016SW001458][[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)}
 +
 +
|- USER ENTRY ADD your inputs in blocks such as the following
 +
|2013-07-09T15:09 UT
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| N20E15 prominence
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| 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
 
|
 
|
 
| N. Savani (neel.savani@nasa.gov)}
 
| N. Savani (neel.savani@nasa.gov)}

Revision as of 13:23, 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. [1]CCMC donki details Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [2]10.1002/2015SW001171

Savani, N. P., Vourlidas, A. et al., 2017, Space Weather, 15: 441 [3]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. [4]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. [5]CCMC donki details Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [6]10.1002/2015SW001171

Savani, N. P., Vourlidas, A. et al., 2017, Space Weather, 15: 441 [7]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. [8]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)}