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Published Materials
Why does the subsolar magnetopause move sunward for radial interplanetary magnetic field?, Samsonov, A. A., Z. Němeček, J. Šafránková, and K. Jelínek, J. Geophys. Res., 117, A05221 (Paper, 10.1029/2011JA017429)

Run Metadata
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Model Domain:GM
Model Name:BATSRUS
Model Version:v8.01
Keywords:radial IMF
 
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:auroral
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:5.00000 n/cc
  SW Temperature:240000.00000 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:-4.99000 nT
  IMF By:0.00000 nT
  IMF Bz:0.32000 nT
  IMF |B|:5.00000 nT
  IMF Clock Angle:0.00000 °
 
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