Paul_Hick_020704_SH_1

Title/Introduction: The magnetic field at the outer boundary will be used as input for a heliospheric tomography model. The main objective is to compare how using the MHD source surface compares with the current purely magnetic (Stanford) source surface models we use as input to the tomography.

Key Word: Source surface magnetic field

Model Type: Solar
Model: MAS
Run Type Type: Relaxation to Steady State
Carrington Rotation: 1956
Coronal Base Density [10⁸ n/cc]: 2
Coronal Base Temperature [10⁶ K]: 1.6
Simulation Grid: low-resolution (61x51x32)
Radial grid range: 1 - 20
Lundquist Number: 1000
Viscosity: 0.05

• View Magnetogram input data
• Read Input file
• Read output file occmc
  
• Plot output file hccmc
• Plot output file qccmc
• Plot output file vccmc
• View 3D Corona

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