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Published Materials
Large-scale flow vortices following a magnetospheric sudden impulse, Samsonov, A. A., and D. G. Sibeck, J. Geophys. Res. Space Physics (Paper, 10.1002/jgra.50329)

Transient changes in magnetospheric-ionospheric currents caused by the passage of an interplanetary shock: Northward interplanetary magnetic field case, Samsonov, A. A., D. G. Sibeck, and Y. Yu, J. Geophys. Res., 115, A05207 (Paper, 10.1029/2009JA014751)

Run Metadata
Metadata as JSON:View Full Run Metadata as JSON
 
Model Domain:GM
Model Name:BATSRUS
Model Version:v7.73
Key Word:interplanetary shock
 
Run type:Simulation with modeled conditions
Inflow Boundary Conditions:Time-dependent
Start Time:2000/01/01 00:00
End Time:2000/01/01 00:01
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:uniform(p=5,h=5)
Radio Flux 10.7 cm:150.
Co-rotation:No corotation velocity is applied at the inner boundary
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:-1.71000 nT
  IMF By:0.00000 nT
  IMF Bz:4.69850 nT
  IMF |B|:5.00000 nT
  IMF Clock Angle:0.00000 °
 
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Output Data

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