JOHAN_MÉNDEZ_082817_SH_2
Key Word: The aim of this simulation is research the influence of the helicity in a 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: 2011
Start Mon: 08
Start Day: 04
Start Hour: 08
Start Min: 47
Poynting ratio: 1.0e6
Coronal Heating: 1.5e5
GL Flux Rope Parameters
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Longitude: 302
Latitude: 17
FR_orientation: 357.02
FR_radius: 0.3
FR_bstrength: -6.72
Cone opening angle:
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Longitude: 10.17
Latitude: 5.09
CME speed: 431
CME traveling time in corona: 48724
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: