---------------------------------------------------------- Reports of the 6 December GEM WG Meetings in San Francisco ---------------------------------------------------------- WG5: GGCM WORKING GROUP Co-chairs: Joel Fedder and George Siscoe The inaugural meeting of the GGCM Working Group (GGCM-WG) was held on December 6, 1992, together with the meetings of the other GEM Working Groups, which were held in conjunction with the Fall AGU Meeting in San Francisco. The meeting had three objectives: 1. Review the generic types of GGCM's as a first step toward optimizing GEM's role in their development; 2. Identify GEM Milestones--relatively short duration, high-impact projects that can be implemented through the GEM program and that contribute to the overarching goal of the program; and 3. Discuss GGCM-WG organizational matters. There were three invited talks on GGCM types. Dick Wolf reviewed the Rice Convection Model (RCM) as an example of a modular GGCM. Joel Fedder pointed out the strengths of global MHD models. Dan Swift described a global hybrid code--kinetic ions/fluid electrons--being developed to run on MPP architecture computers. The detailed reports on the three presentations will be published on The GEMstone soon. The discussion on GEM Milestones project brought to light the possibility of uniting the magnetic field of a global MHD code with the particle drift code of the RCM. This would address major shortcomings of each approach: the RCM's magnetic field is not self-consistently determined, and an MHD model has no gradient and curvature drift features and processes. Dick Wolf and Joel Fedder agreed to look into how such a combined model might be implemented. Another GEM-MP had already been defined at the Snowmass Workshop. Stahara and Spreiter are in contact with Joachim Birn to look at the possibility adding Birn's MHD plasma sheet model with Spreiter and Stahara's vacuum Chapman-Ferraro model with tail. The meeting was highly informative; it generated many useful discussions; and it left the GGCM-WG coordinators with much to do to assimilate the material and prepare for the next Snowmass Workshop.