HR: 0800h
AN: SH11A-0258    [Abstracts]
TI: A 3D Numerical Toolkit for Modeling the Heliosphere
AU: * Spicer, D S
EM: daniel.s.spicer@nasa.gov
AF: NASA/GSFC, Laboratory for Solar and Space Physics, Code 612.1, Greenbelt, MD 20771 United States
AU: Davila, J M
EM: joseph.m.davila@nasa.gov
AF: NASA/GSFC, Laboratory for Solar and Space Physics, Code 612.1, Greenbelt, MD 20771 United States
AU: Ofman, L
EM: ofman@waves.gsfc.nasa.gov
AF: THE CATHOLIC UNIVERSITY OF AMERICA, Institute for Astrophysics and Computational Sciences in The Department of Physics , Washington, DC 20064 United States
AB: We present results from a numerical toolkit that can be used by observers, analysts, and modelers to study solar activity and its effect on the heliosphere. The core of the toolkit is a 3D AMR unstructured mesh high order Godunov code that was orginally designed to model the magnetospheric-ionospheric system. We plan to make the code available in portable code form through the CCMC.
DE: 7513 Coronal mass ejections (2101)
DE: 7519 Flares
DE: 7524 Magnetic fields
DE: 7526 Magnetic reconnection (2723, 7835)
SC: SPA-Solar and Heliospheric Physics [SH]
MN: Fall Meeting 2005