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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)
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
Longitude: 302
Latitude: 17
FR_orientation: 357.02
FR_radius: 0.3
FR_bstrength: -6.72

Cone opening angle:
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
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
Synthetic LASCO C3 coronagraph brightness movie

ASCII files with timelines (plasma parameters) at planets/satellintes:

National Aeronautics and Space Administration Air Force Materiel Command Air Force Office of Scientific Research Air Force Research Laboratory Air Force Weather Agency NOAA Space Environment Center National Science Foundation Office of Naval Research

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