Yi-Hsin_Liu_082016_1c
Title/Introduction: MMS Event DR event
Key Word: MMS Event DR event
Model Type: GM
Model: SWMF version v20140611
Inflow Boundary Conditions:
Start Time: 2015/09/19 05:30
End Time: 2015/09/19 09:40
Dipole Tilt at Start in X-Z Plane: -8.68 deg.
Dipole Tilt in Y-Z GSE Plane: -25.29 deg.
Dipole Update With Time: yes
Ionospheric Conductance: auroral
Radio Flux 10.7 cm: 106.70000
Grid: 4.7M cells, 1/4 Re resolution at the dayside
Coordinate System for the Output: GSM
- View solar wind input data
- List solar wind input data in ASCII format (see format description here).
- View Magnetosphere
- View Magnetosphere (New: simplified, interactive visualization form, currently in beta)
- Create Timeseries in Magnetosphere
- View 2D Ionosphere Electrodynamics
- New: Create Timeseries in 2D Ionosphere
- 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
- Ionospheric dissipation
- View Magnetic perturbation calculated for magnetometer stations:
AAA AAE ABG ABK AIA ALE ALT AMS AND API AQU ARS ASC ASP BDV BEL BFE BFO BLC BMT BNG BOU BOX BRW BSL CBB CLF CMO CNB CNH CSY CTA CZT DED DLR DMC DOB DON DOU DRV DUR EBR ESK EYR FCC FRD FRN FUR GCK GDH GLN GNA GUA GUI GZH HAD HAN HBK HER HLP HON HOP HRB HRN HUA HYB IPM IQA IRT ISK IVA IZN JCK KAK KAR KAU KDU KEV KIL KIR KIV KMH KNY KOU LEK LER LNP LOV LOZ LRM LVV LYC LYR LZH MAB MAS MAW MBC MBO MCQ MEA MEK MGD MID MMB MUO NAL NAQ NCK NEW NGK NOR NUR NVS OTT OUJ PAF PAG PBQ PEG PEL PHU PPT PST QSB RES RVK SBA SFS SHU SIT SJG SNK SOD SOR SPT STJ SUA TAM TAN TAR TDC TEO THL THY TIK TRO TRW TSU TUC UPS VAL VIC VSS WMQ WNG YAK YKC - View model outputs along satellite trajectories (files generated by model at requested, usually short time cadence):
- 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)
This interface has been recently updated. If you experience problems or have any questions please contact the CCMC staff.
