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			 **   THE GEM MESSENGER   **
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						     Volume 12, Number 10
						     May 16, 2002
						     
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Descriptions for the Inner Magnetosphere/Storms Campaign Working Group 1 
Sessions on Ring Current and Plasmasphere at 2002 GEM Telluride Workshop
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From:  Mike Liemohn (liemohn at umich.edu)
       Dennis Gallagher (Dennis.Gallagher at msfc.nasa.gov)

Please find below descriptions for the Working Group 1 (Ring Current and
Plasmasphere) sessions of the Inner Magnetosphere/Storms Campaign at this
summer's GEM Workshop.  We are currently soliciting presentations for any
of these sessions and for the Tuesday night poster session (which includes
these topics as well as presentations on all other IM/S-related issues).
Requests for oral presentations should be sent directly to the session
chairs, while requests for poster presentations should be submitted at the
Workshop website:

    http://koala.rice.edu/~gem/gem2002/gem2002.html

Please note the housing deadlines (May 17 for 2 hotels, June 1 for the
other) and other important dates.  We will try our best to accommodate
everyone in their preferred session, but please keep in mind that some
shifting may be necessary.

      Inner Magnetospheric Magnetic and Electric Fields (joint WG1/WG2)
      Chairs:  Anthony Chan (anthony-chan at rice.edu)
               Mike Liemohn (liemohn at umich.edu)
      Time: Monday, 10:40 am to 12:10 pm

Recently, there have been numerous advances in understanding the perturbed
state of the inner magnetospheric magnetic and electric fields during
storms.  In this session, speakers will present results from a variety of
techniques demonstrating the progress made thus far and highlighting the
progress yet to be made.  The session will primarily focus on magnetic
field structure and dynamics, while most of the electric field discussion
will be reserved for the afternoon session.

     Near-Earth Electric Fields
     Chairs: Jerry Goldstein (jerru at rice.edu)
             Mike Liemohn (liemohn at umich.edu)
     Time: Monday, 1:30 to 3:00 pm

Electric fields develop over large and small scales throughout the inner
magnetosphere.  The objective of this session is to explore their sources,
properties, and effects.

     Empirically Determined Plasmaspheric Structures
     Chairs:  Dennis Gallagher (dennis.gallagher at msfc.nasa.gov)
              Richard Denton (denton at comet.dartmouth.edu)
     Time: Monday, 3:30 to 5:30 pm

Talks will present science results relating to derived magnetospheric
densities and distributions.  Here the talks focus not on the techniques,
but instead on results from use of the various techniques.  The idea is to
cleanly separate technique talks from science results, so both receive
appropriate emphasis.

     Techniques of Detecting Magnetospheric Density
     Chairs: Mark Moldwin (mmoldwin at igpp.ucla.edu)
             Peter Chi (pchi at igpp.ucla.edu)
     Time: Tuesday, 10:30 am to 12:00 pm

Talks in this session will detail the new and improved techniques developed
in recent years to determine magnetospheric densities and distributions.
The intent is to bring everyone up to speed on the capabilities,
assumptions, and limitations of these techniques.  While presentations on
any technique are welcome, special emphasis is placed on remote-sensing of
the inner magnetosphere using networks of ground-based magnetometers.

     Inter-System Coupling: Observations
     Chairs: Pontus C:son Brandt (pontus.brandt at jhuapl.edu)
             Dennis Gallagher (dennis.gallagher at msfc.nasa.gov)
     Time: Tuesday, 1:30 to 3:00 pm

The ionosphere, plasmasphere, superthermal electrons, ring current, and
radiation belts all exhibit interactions that mutually effect their
populations.  This session will focus on those observations that show
evidence of interactions between these regions and populations.  These are
the physical properties in the inner magnetosphere for which theoretical
explanations are sought.

     Inter-System Coupling: Modeling
     Chairs: Mike Liemohn (liemohn at umich.edu)
             Anthony Reynolds (mark.reynolds at erau.edu)
     Time: Tuesday, 3:30 to 5:30 pm

The ionosphere, plasmasphere, superthermal electrons, ring current, and
radiation belts all exhibit interactions that mutually effect their
populations.  This session will focus on those theories that describe the
interactions between these regions and populations.  Emphasis will be placed
on presentations that demonstrate the results of coupling population models.
How these theories can or are used to address relevant observations will be
discussed.  Observations that are needed to advance and test theories will
also be discussed.  It is in this session that we can also invite talks
directed toward the storm Campaign times.

      The magnetosphere and ionosphere under extreme conditions: 
      Points of contact between global MHD simulations and IMS modeling
      and data(joint WG1/WG2, and GGCM)
     Chairs:  George Siscoe (siscoe at bu.edu)
              Janet Kozyra (jukozyra at umich.edu)
     Time: Wednesday, 10:30 am to 12:00 pm

MHD simulations are coming up with some possibly interesting results that
bear on the inner magnetosphere during storm-time conditions.  For example,
all codes seem to show saturation of the polar cap potential for high solar
wind driving electric field.  Some codes also show large parallel
potentials that might draw ions out of the ionosphere and raise them to
ring-current energies, thus possibly supplying the ring current.

     WG1 Wrap-Up:  Progress and Possibilities  (joint WG1/WG2)
     Chairs:  Dennis Gallagher and Mike Liemohn
     Time: Wednesday, 1:30 to 3:00 pm

This session is devoted to discussing the status and direction of WG1
research.  An attempt will be made to quantify and compare the results from
the sessions above, and comprise a list of open/unresolved questions for the
community to consider as part of their future research projects.

      WG2 Wrap-Up. Overflow, Summary, Future Plans (joint WG1/WG2)
      Chairs: Geoff Reeves and Richard Thorne
      Time: Wednesday, 3:30 to 5:30 pm

This session is devoted to discussing the status and direction of WG2
research.

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