HR: 08:45h
AN: SA41B-04    [Abstracts]
TI: Space Weather Modeling Framework: An Overview and Application to the October 29, 2003 Storm
AU: * Ridley, A J
EM: ridley@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Gombosi, T
EM: tamas@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Toth, G
EM: gtoth@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Sokolov, I V
EM: igorsok@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: De Zeeuw, D
EM: darrens@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Chesney, D
EM: chesneyd@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Volberg, O
EM: volov@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Powell, K
EM: powell@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Stout, Q
EM: qstout@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Hansen, K
EM: kenhan@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AU: Kane, K
EM: kanek@umich.edu
AF: University of Michigan, Center for Space Environment Modeling, Ann Arbor, MI 48109-2143 United States
AB: The University of Michigan's Space Weather Modeling Framework (SMWF) aims at providing framework for physics based space weather simulations, as well as for various space physics applications. The SWMF combines numerical models of the Solar Corona, Inner Heliosphere, Solar Energetic Particles, Global Magnetosphere, Inner Magnetosphere, Radiation Belts, Ionosphere and Upper Atmosphere into a parallel, high performance model. We present SWMF results from the October 29, 2003 storm, in which the global magnetosphere (BATSRUS), inner magnetosphere (RCM), ionospheric electrodynamics, and upper atmospheric models (GITM) are run together driven by data from the upstream ACE satellite. We will present comparisons between the simulation results and data from different magnetospheric satellites. We will further present model comparisons between the global magnetosphere run with and without the inner magnetosphere coupling.
DE: 2431 Ionosphere/magnetosphere interactions (2736)
DE: 2447 Modeling and forecasting
DE: 2753 Numerical modeling
DE: 2784 Solar wind/magnetosphere interactions
DE: 2788 Storms and substorms
SC: SPA-Aeronomy [SA]
MN: 2004 AGU Fall Meeting