Run Status: Run Complete
Status updated: 2024-01-06T20:32:22+0000
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 |
Model Domain: | GM |
Model Name: | LFM |
Model Version: | LTR-2_1_5 |
Title/Introduction: | Sept12_2000 |
Key Word: | weak |
Run type: | Real event simulation |
Inflow Boundary Conditions: | Time-dependent |
Start Time: | 2000/09/12 11:00 |
End Time: | 2000/09/13 13:00 |
Dipole Tilt at Start in X-Z Plane: | 5.62 ° |
Dipole Tilt in Y-Z GSE Plane: | -33.55 ° |
Dipole Update With Time: | yes |
Ionospheric Conductance: | auroral |
Radio Flux 10.7 cm: | 134.2 |
Co-rotation: | Corotation potential is being applied |
Grid: | 106x96x128 cells |
Coordinate System for the Output: | SM |
Solar wind input source: | OMNI |
Ring current model: | RCM |
- View pre-computed timeseries data:
- 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
- Ionospheric dissipation
- 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)
- TIE-GCM (2)
- [2000-09-09 - 2000-10-10] Rob_Redmon_011012_IT_1
- [2000-09-01 - 2000-09-29] aswathy_anju_103019_IT_3
SWMF (1)- [07:15 - 2015/12/25 09:00] Katariina_Nykyri_072817_1
NRLMSIS (1)- [2000-01-01 - 2000-12-30] Inkwan_Park_081023_IT_1
MAS (1)- [2000/09/02 23:33 - 2000/09/30 06:01] YuanKuen_Ko_033006_SH_2
LFM (1)- [2000/09/12 11:00 - 2000/09/13 13:00] Adam_Liebers_110723_11
IRI (6)- [2000-01-10 - 2001-01-01] Ali_Uqaily_042724_IT_2
- [2000-01-01 - 2000-12-30] DOHYEON_LEE_100824_IT_5
- [2000-01-01 - 2000-12-30] Fung_Jap_070621_IT_20
- [2000-01-01 - 2000-12-30] Mohit_Jagne_062223_IT_1
- [2000-01-01 - 2000-12-30] Prajakta_Chougule_102323_IT_15
- [2000-08-28 - 2000-10-26] veera_g_031721_IT_5
ENLIL (11)- [2000/09/03 00:05 - 2000/09/13 00:06] Christina_Henning_062510_SH_3
- [2000/09/11 00:07 - 2000/09/21 00:00] Christina_Henning_062510_SH_4
- [2000/09/11 00:07 - 2000/09/21 00:03] Christina_Henning_070810_SH_2
- [2000/09/03 03:36 - 2000/09/30 10:14] Christina_Lee_111606_SH_3
- [2000/09/03 03:36 - 2000/09/30 10:13] Eyob_Talew_062912_SH_5
- [2000/09/03 03:40 - 2000/09/30 10:15] Eyob_Talew_062912_SH_5a
- [2000/09/03 03:40 - 2000/09/30 10:17] Hank_Garrett_052711_SH_65
- [2000/09/02 00:03 - 2000/09/23 00:02] Jin_congqing_053018_SH_8
- [2000/09/10 00:02 - 2000/09/20 00:02] Matthew_Jacobs_061413_SH_1
- [2000/09/10 00:02 - 2000/09/20 00:02] Matthew_Jacobs_061413_SH_2
- [1995/09/02 00:00 - 2000/12/16 00:02] victor_Larraga_040218_SH_3
Similar RunsClick to expand and modify similarity search criteria