Note: CMIT-LFM simulation runs submitted before October 31, 2018 used solar wind data propagated to the model run's upstream (sunward) boundary (typically at Xmax=30 RE).
However, the model assumes solar wind to be propagated to X=0 instead, causing features in the solar wind to occur in the LFM model simulation a few minutes earlier than expected (for example, 8 minutes earlier for Vx=-400 km/s and Xmax=30 RE).
The propagation has been adjusted in the run request system for "event" runs with CMIT-LFM where solar wind data are obtained automatically from one of the available solar wind monitor spacecraft or data sources (solar wind data in uploaded file are not propagated and need to be adjusted before file upload to make LFM runs comparable to runs of the other magnetosphere models).
|Metadata Record:||View Full Run Metadata in the CCMC Metadata Registry (CMR)|
|Metadata as JSON:||View Full Run Metadata as JSON|
|Key Word:||dB/dt R2O Challenge 2011|
|Run type:||Real event simulation|
|Inflow Boundary Conditions:||Time-dependent|
|Start Time:||2005/08/31 10:00|
|End Time:||2005/09/01 12:00|
|Dipole Tilt at Start in X-Z Plane:||0.00 °|
|Dipole Tilt in Y-Z GSE Plane:||0.00 °|
|Dipole Update With Time:||yes|
|Co-rotation:||Corotation velocity is applied at the inner boundary.|
|Coordinate System for the Output:||SM|
|Initial Solar Wind (SW) Parameters in SM Coordinates:|
|SW Density:||17.56000 n/cc|
|SW Temperature:||33015.70000 Kelvin|
|X Component of SW Velocity:||-412.96000 km/s|
|Y Component of SW Velocity:||-7.67000 km/s|
|Z Component of SW Velocity:||62.26000 km/s|
|IMF Bx:||0.00000 nT|
|IMF By:||16.45000 nT|
|IMF Bz:||3.06000 nT|
|IMF |B|:||16.73000 nT|
|IMF Clock Angle:||79.50000 °|
- Pre-computed time series outputs not available
- View model outputs along satellite trajectories (result of postprocessing on usually longer magnetosphere 3D output time cadence):
- Perform model data comparison for this run using VMR tools (formerly the Virtual Model Repository at the University of Michigan)
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