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).

Run Metadata
Metadata as JSON:View Full Run Metadata as JSON
 
Model Domain:GM
Model Name:LFM
Model Version:LTR-2_1_5
Title/Introduction:Dual Auroras
Key Word:Dual Auroras
 
Run type:Simulation with modeled conditions
Inflow Boundary Conditions:Time-dependent
Start Time:2001/08/17 10:00
End Time:2001/08/17 10:00
Dipole Tilt at Start in X-Z Plane:12.46 °
Dipole Tilt in Y-Z GSE Plane:-29.78 °
Dipole Update With Time:yes
Ionospheric Conductance:auroral
Radio Flux 10.7 cm:148.4
Co-rotation:Corotation potential is being applied
Grid:low_mach grid with 53x48x64 cells
Coordinate System for the Output:SM
Solar wind input source:ACE-L2
Initial Solar Wind (SW) Parameters in SM Coordinates:
  SW Density:18.78700 n/cc
  SW Temperature:19145.90000 Kelvin
  X Component of SW Velocity:-344.83300 km/s
  Y Component of SW Velocity:7.98000 km/s
  Z Component of SW Velocity:15.47400 km/s
  IMF Bx:-0.85800 nT
  IMF By:4.06100 nT
  IMF Bz:1.35900 nT
  IMF |B|:4.28000 nT
  IMF Clock Angle:71.50000 °
 
Input Data
  • View solar wind input data
  • List solar wind input data in ASCII format (see format description here).
    • Output Data
  • View Magnetosphere
  • Create Timeseries in Magnetosphere
  • View 2D Ionosphere Electrodynamics
  • New: Create Timeseries in 2D Ionosphere

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