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Do we know the actual magnetopause position for typical solar wind conditions?, Samsonov, A. A., E. Gordeev, N. A. Tsyganenko, J. Šafránková, Z. Němeček, J. Šimůnek, D. G. Sibeck, G. Tóth, V. G. Merkin, and J. Raeder, J. Geophys. Res. Space Physics, 121, 6493–6508 (Paper, 10.1002/2016JA022471)

Run Metadata
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Model Domain:GM
Model Name:OpenGGCM
Model Version:4.0
Title/Introduction:TEST Parker
Keywords:Parker spiral
 
Run type:Simulation with modeled conditions
Inflow Boundary Conditions:Time-dependent
Start Time:2000/01/01 00:00
End Time:2000/01/01 04:00
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:7M dayside
Coordinate System for the Output:GSE
Solar wind input source:user-uploaded
Initial Solar Wind (SW) Parameters in GSE Coordinates:
  SW Density:5.00000 n/cc
  SW Temperature:200000.00000 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:-3.53500 nT
  IMF By:0.00000 nT
  IMF Bz:-5.00000 nT
  IMF |B|:5.00000 nT
  IMF Clock Angle:180.00000 °
 
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