Brad Hindman (JILA/University of Colorado). Invited speakers (afternoon): David Alexander (Rice University) Chip Manchester (University of Michigan). Active Region Magnetic Fields: From the Photosphere to the Corona.
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Invited speakers (afternoon):
David Alexander (Rice University)
Chip Manchester (University of Michigan)
Masahito Kubo (HAO/NCAR): Magnetic flux budget of a decaying sunspot
inner area Corona
Outside moat region
Brad Hindman (JILA/University of Colorado): Subsurface circulations established by active regions
Plage circulations established by active regions
(depth < 2 Mm)
(depth < 7 Mm)
(depth > 10 Mm)
David Alexander (Rice University): Inferences from observations of active region flux
FOLLOWING POLARITY (*) SHOWS MORE FLUCTUATION
HELICITY IS ASYMMETRIC
d: total helicity flux (x1042Mx2) over 5 days for the positive and negative polarities
c: helicity injection rate (x1040Mx2 per hr) the positive and the negative polarities
Chip Manchester (University of Michigan): the dynamics and evolution of the sub-surface expectations?
Study of flux emergence: Photospheric shear flows that produce coronal eruptions
Shine session proposal: the dynamics and evolution of the sub-surface expectations?
Observations and modeling of the theoreticians active region,
subphotosphere to corona
New cycle active region case studies
Submit results for session