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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

Synthetic coronagraph images (individual frames):

Synthetic LASCO C2 coronagraph movies:

base difference
Synthetic LASCO C2 coronagraph base difference movie		 running difference
Synthetic LASCO C2 coronagraph running difference movie		 brightness
Synthetic LASCO C2 coronagraph brightness movie


Synthetic LASCO C3 coronagraph movies:

base difference
Synthetic LASCO C3 coronagraph base difference movie		 running difference
Synthetic LASCO C3 coronagraph running difference movie		 brightness
Synthetic LASCO C3 coronagraph brightness movie