Sarah_Gibson_080905_SH_1

Title/Introduction: We have chosen this interval because we wish to compare MAS predictions to observations of coronal magnetic fields taken by the HAO/NCAR Coronal Multichannel Polarimeter (COMP).

Key Word: COMP

Model Type: Solar
Model: MAS
Run Type Type: Relaxation to Steady State
Carrington Rotation: 2029
Coronal Base Density [10⁸ n/cc]: 2
Coronal Base Temperature [10⁶ K]: 1.6
Simulation Grid: medium resolution (85x81x64)
Radial grid range: 1 - 30
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