AM I: 08:30 - 10:00
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Pre-Event Reconnection and Current Sheet Formation (Hosted by WG2)
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Break, posters |
AM II: 10:30 - 12:00
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A Debate (Hosted by WG1):
Resolved: Eruptive Flares and CMEs are initiated by the helical kink instability
Pro:
Fan, Y. |
Numerical simulations of 3D coronal magnetic fields resulting from
the emergence of twisted magnetic flux tubes |
Rust, D. |
Observations of eruptions |
Con:
Titov, V. |
Numerical simulations of the eruption of twisted flux |
Canfield, R. |
Observations of ARs and sigmoids in the photosphere and corona |
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Lunch |
PM I: 13:30 - 15:00
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WG1 Mini-Groups (in parallel)
WG1a: Inferring velocity fields from magnetograms
Organizer: B. Welsch
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WG1b: Open session
Organizer: R. Canfield
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Kusano, K. |
tbd |
Leka, K. |
Twist, kink, and other contortions |
Longcope, D. |
tbd |
Pevtsov, A. |
Role of trans-equatorial loops in eruptions |
Georgeolis, M. |
tbd |
Morita, S. |
Properties of a flare productive magnetic polarity inversion line:
its genesis and decay |
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Break, posters |
PM II: 15:30 - 17:30
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WG1 mini-groups (WG1a and WG1b) in parallel, 15:30 - 16:30
WG1a: Inferring velocity fields from magnetograms (continued)
Organizer: B. Welsch
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WG1b: Open session (continued)
Organizer: R. Canfield
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Welsch, B. |
tbd |
Kuhn, J. |
Infrared coronal magnetometry |
Schuck, P. |
tbd |
Barnes, G. |
Tests of the force-free state of the photosphere and chromosphere |
WG1 Wrap-up (all of WG1 meets together, 16:30 - 17:30):
Open Discussion: What did we learn at this workshop?
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Reception |