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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:SWMF
Model Version:v8.01
Title/Introduction:Magnetospheric Reconnection, clock 180, density 5
Key Word:Reconnection, Resistivity, High res, Lower Density
 
Run type:Simulation with modeled conditions
Inflow Boundary Conditions:Time-dependent
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:constant
Radio Flux 10.7 cm:0.00000
Co-rotation:No corotation velocity is applied at the inner boundary
Grid:low_mach ck1
Coordinate System for the Output:GSM
Solar wind input source:user
Initial Solar Wind (SW) Parameters in GSM Coordinates:
  SW Density:5.00000 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 °
Magnetosphere Run Parameters:
  GM solver:Rusanov
  GM limiter name:minmod
  GM limiter beta:1
  GM implicit:explicit
  GM Boris clight factor:0.01
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