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			 **   THE GEM MESSENGER   **
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						     Volume 5, Number 40
						     December 20, 1995

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           Brief Report on the Fall 1995 NSF/GEM Mini-Workshop

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                           Harlan E. Spence
                        GEM Meetings Coordinator
                Boston University Center for Space Physics


     The Fall 1995 National Science Foundation (NSF) Geospace Environment
Modeling (GEM) mini-workshop was held on Sunday, December 10, 1995,  in San
Francisco, CA.   Each year GEM convenes this one-half-day mini-workshop on
the Sunday preceding the American Geophysical Union Fall Meeting, as a
supplement to the full one-week summer GEM workshop held traditionally at
the end of June in Snowmass, CO.  The Fall mini-workshop is designed
primarily for those GEM working groups requiring discussions and/or
planning on a semi-annual basis.   Over 75 scientists participated in this
year's mini-workshop which lasted from 1:00 to 7:00pm at the Moscone
Center.

    The NSF/GEM program is a phased, multi-campaign effort, now in its
fifth year of funding.  Each of the active and planned campaigns is aimed
at understanding and describing the physics of a particular region of
geospace by: coordinating the collection and analysis of both ground- and
space-based measurements relevant to that region;  developing quantitative
physical or empirical models of these regions; and testing, assessing, and
refining the models.  Each region-specific campaign interacts with the
Geospace General Circulation Model  (GGCM) campaign, which is collecting
campaign models and synthesizing them into a modularized, global model.  At
present, the GEM program has two active region-specific campaigns:  the
Boundary Layer (BL) campaign on the physics of the magnetopause and its
associated boundary layers; and the Tail/Substorm (TS) campaign on the
physics of the geomagnetic tail under both geomagnetically quiescent and
active conditions.  Each of the three ongoing campaigns is comprised of
three working groups.  Each working group has a distinct task toward the
campaign goal and whose focus is provided either by science topic or
technique.

   Three of the possible nine working groups (WGs) met this year and their
synopses follow:

 --- The BL WG#1 ("Reconnection Electric Field and Magnetopause Boundary
Normal Magnetic Field") is co-chaired by Lawrence Lyons of The Aerospace
Corporation and Alan Rodger of the British Antarctic Survey.  This working
group is exploring the ionospheric and magnetospheric signatures of the
boundary between open and closed magnetic field lines using a variety of
coordinated data sources.  The BL WG#1 agenda included: brief progress
reports of ongoing projects since the summer 1995 Snowmass meeting;
identification of candidate study periods from recently acquired data;
planning for the 1996 Snowmass meeting; and definition of future campaign
dates.

 --- The BL WG#3 ("Current Systems and Mapping") is co-chaired by Eigil
Friis-Christensen of the Danish Meterological Institute and Nancy Crooker
of Boston University.  This working group is studying
high-magnetic-latitude current systems and their mapping from the
ionosphere to the magnetosphere.  The BL WG#3 agenda was mainly
programmatic, including: discussion of working group objectives;
assessment of progress toward achieving goals; and exploration of future
working group directions.

 --- The TS WG#1 ("Substorm Onset Signatures: Identification, Location, and
Timing") is co-chaired by  Nelson Maynard of Mission Research and Lawrence
Lyons. Agenda highlights for  TS WG#1 included: review of magnetic field
and current configurations measured by the CRRES satellite; description of
data sets of two recent event periods acquired through coordination with
the International Solar Terrestrial Physics (ISTP) program; and discussion
of future GEM/ISTP coordinated observations.

     The final session of the workshop, chaired by Delores Knipp of the
United States Air Force Academy, focused on the "Space Weather Event of 3-5
November 1993."  The goal of this initiative is to follow a significant
solar-terrestrial event from its origin at the Sun and to trace the flow of
particles and energy from the subsequent magnetic storm through the
dissipative elements of the magnetosphere, ionosphere, and thermosphere.
The agenda included a review of the vast amount of data collected and
discussion of the data analysis and synthesis that is underway.  This
session involved not only the GEM community, but also scientists
representing other NSF-sponsored programs in aeronomy (CEDAR - Coupling,
Energetics, and Dynamics of Atmospheric Regions) and solar-heliospheric
physics (SHINE - Solar, Heliospheric, and INterplanetary Environment), who
had met separately at the Moscone Center earlier in the day.  A future
joint GEM/CEDAR/SHINE meeting is planned as a part of next summer's
workshop agendas.

     For an update on other GEM working group activities, I invite you to
browse the GEM World Wide Web Home Page (managed by Chris Russell and Guan
Le of UCLA) at "http://www.ucla.edu.spa.gem".  At this site, you will find
links to an extensive amount  of detailed material on the GEM program
including complete working group reports, steering committee reports, and
current and back-issues of The GEM Messenger - the electronic GEM
newsletter. You will also discover a novel GEM experiment called the GEM
"Virtual" On-line Poster session, where GEM-relevant posters may be viewed
electronically.

   Warm wishes for a healthy and happy holiday!

                        Best regards, --- Harlan E. Spence

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Harlan E. Spence
Asst. Professor of Astronomy
Center for Space Physics and Department of Astronomy
College of Liberal Arts and Graduate School of Arts and Sciences
Boston University
725 Commonwealth Avenue
Boston, MA  02215
Ph:     (617) 353-7412
Fax:    (617) 353-6463
e-mail:  spence at bu.edu
WWW:     http://bu-ast.bu.edu/people/spence.html
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