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			 **   THE GEM MESSENGER   **
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						     Volume 5, Number 40
						     December 21, 1995

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Update on GEM GGCM Campaign/SEC Space Weather Workshop
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From: George Siscoe (siscoe at buasta.bu.edu)

GEM GGCM Campaign/SEC Space Weather Workshop
January 11-12, 1996
       and
Pre-Snowmass Workshop 
January 13, 1996
Space Environment Center
Boulder, Colorado

This is an update on the GEM GGCM Campaign/SEC Space Weather 
Workshop.  The agenda is slightly but interestingly modified. 
This is also an announcement of an extra day added to the 
workshop to give the GGCM Campaign time to plan its response to a 
challenge put forth by the GEM Boundary Layer Campaign, which is to 
model from solar wind/IMF inputs the results of their campaigns.  All 
modelers interested in responding to the challenge are invited to 
stay for the Saturday session.  The specific details of the challenge 
will then be revealed.  The time will be spent defining tasks to be 
completed in time for a presentation at the Snowmass workshop. An agenda 
for the Saturday session will be distributed in a separate newsletter.

Agenda for January 11 and 12

Thursday, January 11

08:30 Welcoming Remarks...Ernest Hildner, Director SEC
08:35 Meeting logistics...Howard Singer
08:40 Meeting goals..George Siscoe
08:45 The National Space Weather Program Implementation Plan
      and GEM...Rich Behnke, Director, Upper Atmosphere 
      Research Section, NSF
09:10 Directions for magnetospheric models and sensors:
      An Air Force Perspective...Lt. Col. C. Tschan (50 WS)
09:35 MSM performance at 50th Weather Squadron...Kevin Scro
10:00 Break
10:30 WIND/SWIM: The first L1 space weather station
            Introductory remarks...Bob Carovillano
10:35 Using & distributing real-time SWIM data & thinking ahead 
      to ACE...Kent Doggett (SEC)
10:50 A post-ACE, L1 space-weather station...Pete Bythrow
11:05 Comparing prediction with eventuality: A case study...
      J. Kunches (SEC)
11:20 Harvesting the low hanging fruit: The 1 to 2 year 
      perspective...Howard Singer (SEC)
11:40 Getting ready for Solar Max 23: GEM community 
      opportunities...JoAnn Joselyn (SEC)
12:00 Lunch
01:00 Panel discussion on boundary position specification and 
      forecasts
      Panelists: M. Heinemann (Moderator); K. Doggett;
        J. Lyon; C. Russell; H. Singer; P. Song; 
        S. Stahara/J. Spreiter; D. Vassiliadis
02:30 Break
03:00 Panel discussion on radiation belts
      Panelists:M. Hudson (Moderator); T. Cayton; M. Chen; 
        G. Ginet; X. Li; D. Speich
04:30 Panel discussion on disturbance index forecasts (Kp, K, A, 
      AU, AL, AE, Dst, PC)
      Panelists:R. Wolf (Moderator), T. Detman; J. Fedder; J. Freeman; 
        J. Hirman; J. Joselyn; J. Kozyra; A. S. Sharma
05:30 Adjourn

Friday, January 12

08:30 Panel discussion on auroral electrojet and GIC forecasts
      Panelists: H. Singer (Moderator); C. Balch; G. Erickson; 
        J. Fedder; J. Kappenman; G. Lu; N. Maynard; V. Papitashvili; 
        J. Raeder; D. Vassiliadis; J. Walker; L. Zanetti
10:00 Break with demonstration of Dan Weimer's universal IMF 
            potential pattern algorithm
10:30 Panel discussion on models
      Panelists: G. Siscoe (Moderator); J. Berchem; T. Detman; M. Hesse; 
        J. Fedder; B. Sonnerup; R. McPherron; T. Onsager; J. Raeder; 
        F. Toffoletto; W. White; R. Wolf
12:00 Lunch
01:00 Panel discussion on implementation
      Panelists: R. Behnke (Moderator); R. Carovillano; G. Heckman; 
      E. Hildner; H. Petschek; Capt. A. Preble; K. Scro; 
      Lt. Col. C. Tschan
02:30 Closing discussion...R. Zwickl (Moderator)
03:00 End

Panel discussion format: Each discussion will comprise 5-minute, 
2-vugraph presentations by panelists followed by (prearranged with 
panel moderator) 5-minute, 2-vugraph contributions from the floor 
followed by panel discussion with questions and comments from the 
floor.  Each panel will address the questions: where do we want to 
be in the panel's topic area in 2 years and 5 years? where are we now? 
and what needs to happen to get from here to there?  The question, 
where are we now?, will likely be the subject of the opening 
contributions from the panel and the floor.  There will be additional 
questions specific to each panel, as follows:

Panel on boundary position specification and forecasts: How do we 
build reliable prediction algorithms for extreme events?

Panel on radiation belts: What roles do diffusion, convection,
and surfing play in populating the radiation belts?  What is 
the physics behind the energetic outer electron belt?

Panel on disturbance index forecasts: How do we move beyond the
historical indices to indices appropriate to now?

Panel on auroral electrojet and GIC forecasts: How can we measure
spatiotemporal forecast reliability so that users will know 
when they are reliable enough to justify taking costly actions to 
avoid predicted problems?  Is it useful to think of an optimal mix
of forecast approaches?

Panel on models: What are the prospects for MSFM upgrades--e.g. 
incorporating a Toffoletto/Hill-like module and radiation belt 
modules?  Ditto for Drift-orbit/MHD hybrids?  How do we regulate 
solar wind coupling and substorm dynamics?  Is regulation neces-
sary?  How do we treat real-time data assimilation?  What are the 
operational roles of analytical, semi-empirical, statistical, and 
numerical models?

Panel on implementation: Is there a procedure by which algorithm 
developers (science types) and space weather service officers 
(forecaster types) can bring about diagnosing, specification and 
forecast algorithms that are tested, certified, and transitioned 
into operation?  How can two-way information flow between these 
two groups be established and fostered?  What steps will lead to 
increasing the value of space weather services?

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