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Run Status: Run Complete
Status updated: 2002-10-24T00:00:00+00:00

Published Materials
Field-aligned currents during northward interplanetary magnetic field: Morphology and causes, Vennerstrom, S., T. Moretto, L. Rastätter, and J. Raeder, J. Geophys. Res., 110, A06205 (Paper, 10.1029/2004JA010802)

Run Metadata
Metadata as JSON:View Full Run Metadata as JSON
 
Model Domain:GM
Model Name:UCLA-GGCM
Model Version:2.1-1
Keywords:Slowly rotating IMF
 
Run type:Simulation with modeled conditions
Inflow Boundary Conditions:Time-dependent
Start Time:2000/01/01 0:00
End Time:2000/01/01 2:00
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
Co-rotation:No corotation velocity is applied at the inner boundary
Coordinate System for the Output:GSE
Initial Solar Wind (SW) Parameters in GSE Coordinates:
  SW Density:7.00000 n/cc
  SW Temperature:40000.00000 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:10.00000 nT
  IMF |B|:10.00000 nT
  IMF Clock Angle:0.00000 °
 
Input Data
Output Data

  • Pre-computed time series outputs not available
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