Runs on Request

John_Raymond_033111_SH_2

Title/Introduction: CORHEL model of B field above 3 Rsun This is designed to find the magnetic field, density and temperature to determine the V x B force on dust particles in the tail of sungrazing comet C/2003 K7 observed by LASCO and UVCS.

Key Word: C/2003 K7 sungrazing comet

Model Type: Solar
Model: CORHEL
Run Type Type: Relaxation to Steady State
Carrington Rotation: 1993
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