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Published Materials
Tracing magnetic separators and their dependence on IMF clock angle in global magnetospheric simulations, Komar, C. M., P. A. Cassak, J. C. Dorelli, A. Glocer, and M. M. Kuznetsova, J. Geophys. Res. Space Physics, 118, 4998–5007 (Paper, 10.1002/jgra.50479)

Run Metadata
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Model Domain:GM
Model Name:BATSRUS
Model Version:v8.01
Key Word:Magnetic Reconnection, Resolution 1/8 Re
 
Run type:Simulation with modeled conditions
Inflow Boundary Conditions:Fixed
Start Time:2000/01/01 00:00
End Time:2000/01/01 02:00
Dipole Tilt at Start in X-Z Plane:0.00 °
Dipole Tilt in Y-Z GSE Plane:0.00 °
Dipole Update With Time:no
Ionospheric Conductance:uniformp5,h5
Radio Flux 10.7 cm:150.
Co-rotation:No corotation velocity is applied at the inner boundary
Grid:2M cells
Coordinate System for the Output:GSM
Initial Solar Wind (SW) Parameters in GSM Coordinates:
  SW Density:20.00000 n/cc
  SW Temperature:232100.00000 Kelvin
  X Component of SW Velocity:-400.00000 km/s
  Y Component of SW Velocity:0.00000 km/s
  Z Component of SW Velocity:0.00000 km/s
  IMF Bx:0.00000 nT
  IMF By:0.00000 nT
  IMF Bz:-20.00000 nT
  IMF |B|:20.00000 nT
  IMF Clock Angle:180.00000 °
 
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