Robert_Leamon_042309_SH_1

Title/Introduction: 2003 October 29 To see how different the coronal magnetic field generated from an MHD model compares to a PFSS model, on a (the most!?) active day.

Key Word: Halloween

Model Type: Solar
Model: MAS
Run Type Type: Relaxation to Steady State
Carrington Rotation: 2009
Coronal Base Density [10⁸ n/cc]: 2
Coronal Base Temperature [10⁶ K]: 1.6
Simulation Grid: medium resolution (101x101x128)
Radial grid range: 1 - 30
Lundquist Number: 1000
Viscosity: 0.05

• View Magnetogram input data
• View 3D Corona
• View quick look graphics for the run
• View convergence monitor plot for the run to decide if the run duration for the request was OK