SCD News > Announcement: October 13, 2005
Amitava Bhattacharjee
Space Science Center
Institute for the Study of Earth, Oceans, and Space
University of New Hampshire
Friday, October 28, 2005
1:30 p.m.
Foothills Bldg. 2, Room 1001
Recent developments in the theory of nonlinear collisionless reconnection
hold the promise for providing solutions to some outstanding problems space
and laboratory plasma physics. Examples of such problems are sawtooth oscillations
in tokamaks, magnetotail substorms, and impulsive solar (or stellar) flares.
In each of these phenomena, a long-standing issue has been the identification
of fast reconnection rates that are insensitive to the magnitude of the plasma
resistivity. Furthermore, these phenomena often exhibit a “trigger”---the
magnetic field configuration evolves slowly for a long period of time, only
to undergo a sudden dynamical change over a much shorter period of time.
In
this talk, I will demonstrate that these phenomena can be viewed from a common
theoretical perspective based on a Hall MHD reconnection model. Predictions
of theory and simulation will be compared with observations. I will also report
on some new developments in fully three-dimensional reconnection models of
the magnetosphere and the solar corona.
For more information, contact Liz Rothney at x1351, rothney@ucar.edu
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