Yu_Liu_062807_SH_1

Title/Introduction: The results will supply us with the simulated density and temperature distributions in the 3D corona that is crucial for understanding our solar coronal magnetic field observation.

Key Word: CR2014; Solar Magnetic Field Measurement

Model Type: Solar
Model: MAS
Run Type Type: Relaxation to Steady State
Carrington Rotation: 2014
Coronal Base Density [10⁸ n/cc]: 2
Coronal Base Temperature [10⁶ K]: 1.6
Simulation Grid: low-resolution (61x71x64)
Radial grid range: 1 - 20
Lundquist Number: 1000
Viscosity: 0.05

• View Magnetogram input data
• View 3D Corona
• View 3D heliosphere data
• View quick look graphics for the run