John_Raymond_040811_SH_1

Title/Introduction: Magnetic field for Comet C/2002 S2 The magnetic field at heights between 5 and 10 solar radii will be used to compute the deflection of small charged dust particles to determine whether that can explain unexpected properties of the Ly alpha emission.

Key Word: sungrazing comet C/2002 S2

Model Type: Solar
Model: CORHEL
Run Type Type: Relaxation to Steady State
Carrington Rotation: 1994
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 3D Corona
• View 3D Heliosphere data