Project: 1997-05-12 Interplanetary Event
Summary: Numerical simulation of the interplanetary disturbances generated by the halo CME on 1997-05-12. Heliospheric model is driven by time-dependent boundary conditions derived from the SAIC ambient wind and XPZ cone models. Results are stored as 3-D distributions of parameters at time levels and as temporal evolutions at positions on the Sun-Earth line and the near-Earth points.
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Case - grid 256x30x90, initial/boundary values c1a1b2
Code - grid 256x30x90 , processing element 1, model mcp3mt-1
Run - grid 256x30x90, initial/boundry values c1a1b2, processing element 1, model mcp3mt-1, parameters par1