Run Status: Run Complete
Status updated: 2024-09-12T05:06:02+0000
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: | SH |
Model Name: | SWMF |
Model Version: | AWSoM |
Key Word: | march2022_cme2 |
CME Eruption Time (at the solar surface): | |
Date: | 2022/03/30 00:03 |
Poynting ratio: | 0.5 |
Coronal Heating: | 1.5 |
GL Flux Rope Parameters: | |
Longitude: | 84 |
Latitude: | 12 |
FR_orientation: | 164.58 |
FR_radius: | 0.3 |
FR_bstrength: | -22.33 |
Cone opening angle: | |
Longitude: | 8 |
Latitude: | 4 |
CME speed: | 760 |
CME traveling time in corona: | 27632 |
Smoothing factor: | 5 |
Input Data
- Download Magnetogram file
- Download PARAM.expand.start configuration parameters file
- Download PARAM.expand.restart configuration parameters file
- Download mf.dat
- Download harmonics.dat
Output Data
- Download earth.sat
- Download sta.sat
- Download stb.sat
- View 3D SC Data
- View Timeseries of 3D SC Data
- View 3D IH Data
- View Timeseries of 3D IH Data
![In-situ plasma comparison between observation and model output (STEREOA)](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_CR2255_sta.png)
![In-situ plasma comparison between observation and model output (OMNI)](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_CR2255_omni.png)
![Comparison between model simulations (1st row) and remote sensing observations from STEREOA/EUVI (2nd row)](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_CR2255_los_euvia.png)
![Comparison between model simulations (1st and 2nd rows) and remote sensing observations from SDO/AIA (3rd and 4th rows)](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_CR2255_los_aia_IDL.png)
![test test](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_Br_harmonics_bxyz.png)
![Radial magnetic field from GONG magnetogram](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_Br_fitsfile.png)
![Radial magnetic field input to the MHD model](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_Br_field_2d.png)
![2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in z=0 plane](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_z=0.gif)
![2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in y=0 plane](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_y=0.gif)
![2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in x=0 plane](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_x=0.gif)
![Synthetic LASCO C3 coronagraph brightness movie](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_C3_LOS_WLB_movie.gif)
![Synthetic LASCO C3 coronagraph running difference movie](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_C3_LOS_RDIFF_movie.gif)
![Synthetic LASCO C3 coronagraph base difference movie](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_C3_LOS_BDIFF_movie.gif)
![Synthetic LASCO C2 coronagraph brightness movie](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_C2_LOS_WLB_movie.gif)
![Synthetic LASCO C2 coronagraph running difference movie](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_C2_LOS_RDIFF_movie.gif)
![Synthetic LASCO C2 coronagraph base difference movie](/RoR_WWW/SH/SWMF/2023/Leila_Mays_031023_SH_5/images/Leila_Mays_031023_SH_5_C2_LOS_BDIFF_movie.gif)
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