JOHAN_MENDEZ_062817_SH_2
Key Word: I want to calculate the helicity and its importance in the final CME
Model Type: Solar/Heliosphere
Model: SWMF
Version: AWSoM_R 1.0
CME Eruption Time (at the solar surface)
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Start Year: 2013
Start Mon: 04
Start Day: 18
Start Hour: 20
Start Min: 24
Poynting ratio: 1.0e6
Coronal Heating: 1.5e5
GL Flux Rope Parameters
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Longitude: 343
Latitude: 25
FR_orientation: 359.59
FR_radius: 1
FR_bstrength: 1
Cone opening angle:
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Longitude: 8
Latitude: 4
CME speed: 543
CME traveling time in corona: 38674
Smoothing factor: 5
- View 3D SC Data
- View 3D IH Data
Synthetic coronagraph images (individual frames):
- Synthetic LASCO C2 coronagraph images - base difference
- Synthetic LASCO C2 coronagraph images - running difference
- Synthetic LASCO C2 coronagraph images - brightness
- Synthetic LASCO C3 coronagraph images - base difference
- Synthetic LASCO C3 coronagraph images - running difference
- Synthetic LASCO C3 coronagraph images - brightness
Synthetic LASCO C2 coronagraph movies:
base difference |
running difference |
brightness |
Synthetic LASCO C3 coronagraph movies:
base difference |
running difference |
brightness |
ASCII files with timelines (plasma parameters) at planets/satellintes: