Focus and Scope
This three-day workshop will focus primarily on the latest space-borne and
ground-based observations relevant to the theoretical models of solar
magnetic fields.
Recent instrumentation and analysis techniques have made advances
pertinent to models of the solar dynamo, models of the solar
corona, and models for energy release in solar flares and coronal
mass ejections. For their part, theoretical models have developed
to a level of sophistication that increasingly make it possible to address
observations directly. This workshop will focus on the latest
observational results and discuss the challenges they present for theory
and modeling.
The workshop is intended partly to initiate a separate ten-week
theoretical program focusing on solar magnetic fields and crossover
applications to astrophysics. The topics of the workshop will be
aimed toward stimulating work in the focal areas of the ten-week program:
- The origin and evolution of magnetic fields in the solar interior,
with a particular emphasis on relating the observed fields at the
surface of the Sun to their subsurface properties,
- The role that changing magnetic fields in the corona
play in the explosive release of energy,(with an emphasis
on reconnection and particle acceleration during solar flares),
- how magnetic field evolution at the photospheric level
drives coronal mass ejections and solar wind flows, and
- the application of the lessons learned from the Sun to
other astrophysical environments.
All meeting participants are invited to submit contributed talks in the form of posters, which will be available for viewing during the 3 days of the meeting.
Registration
Please register using the online registration form. The registration fee is $200, due on Dec. 15, 2001(after that date add $50 late fee). The total number of participants is limited, and early registration is recommended to secure your place.
Contact
For further information or questions, please contact Dorene Sexton Iverson, ITP Conference Assistant. |