SWPC_SWMF_022512_7
Run Metadata
| Metadata Record: | View Full Run Metadata in the CCMC Metadata Registry (CMR) |
| Metadata as JSON: | View Full Run Metadata as JSON |
| Model Domain: | GM |
| Model Name: | SWMF |
| Model Version: | v20110131 |
| Title/Introduction: | SWPC Challenge |
| Key Word: | dB/dt R2O Challenge 2011 April 05, 2010, SSW16 |
| Run type: | Real event simulation |
| Inflow Boundary Conditions: | Time-dependent |
| Start Time: | 2010/04/04 19.00 |
| End Time: | 2010/04/06 00:00 |
| Dipole Tilt at Start in X-Z Plane: | -16.11 ° |
| Dipole Tilt in Y-Z GSE Plane: | -28.17 ° |
| Dipole Update With Time: | yes |
| Ionospheric Conductance: | auroral |
| Co-rotation: | No corotation velocity is applied at the inner boundary. |
| Grid: | 1M cells |
| Coordinate System for the Output: | GSM |
| Solar wind input source: | ACE_L2/WIND (user-uploaded) |
| Ring current model: | RCM |
| Initial Solar Wind (SW) Parameters in GSM Coordinates: | |
| SW Density: | 3.72600 n/cc |
| SW Temperature: | 101590.00000 Kelvin |
| X Component of SW Velocity: | 0.00000 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: | -4.06700 nT |
| IMF Bz: | 2.17900 nT |
| IMF |B|: | 4.61000 nT |
| IMF Clock Angle: | -61.82000 ° |
| Magnetosphere Run Parameters: | |
| GM solver: | Sokolov |
| GM limiter name: | mc3 |
| GM limiter beta: | 1.2 |
| GM implicit: | part-implicit |
| GM timestep: | 5.0 |
| GM Boris clight factor: | 0.01 |
Input Data
Output Data
- View pre-computed timeseries data:
- SWMF diagnostic log file with CPCPN (CPCP North), CPCPS (CPCP South), Dst (SymH)
- Northern hemisphere polar cap flux and area
- Southern hemisphere polar cap flux and area
- Magnetopause standoff and closest approach within 30 deg. of Sun-Earth line (local noon)
- Polar cap boundary at 24 magnetic local times in northern hemisphere
- Polar cap boundary at 24 magnetic local times in southern hemisphere not available
- Ionospheric dissipation
- View Magnetic perturbation calculated for magnetometer stations:
- 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)
Run Services
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