Run Status: Run Complete
Status updated: 2024-01-31T19:52:09+0000

Run Metadata
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:2022/03/28 20:23
  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
 
Output Data
Quick Look Graphics (?)
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  • Quick look graphics has been designed by the model developers to enable quick evaluation of the results of the run. To find more information regarding this option please contact the CCMC staff.
In-situ plasma comparison between observation and model output (STEREOA)
In-situ plasma comparison between observation and model output (STEREOA)
In-situ plasma comparison between observation and model output (OMNI)
In-situ plasma comparison between observation and model output (OMNI)
Comparison between model simulations (1st and 2nd rows) and remote sensing observations from SDO/AIA (3rd and 4th rows)
Comparison between model simulations (1st and 2nd rows) and remote sensing observations from SDO/AIA (3rd and 4th rows)
test test
test test
Radial magnetic field from GONG magnetogram
Radial magnetic field from GONG magnetogram
Radial magnetic field input to the MHD model
Radial magnetic field input to the MHD model
2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in z=0 plane
2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in z=0 plane
2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in y=0 plane
2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in y=0 plane
2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in x=0 plane
2d movie of scaled radial magnetic field (Br*r^2) overlaid with magnetic field lines in x=0 plane
MHD MHTIME
MHD MHTIME
Synthetic LASCO C3 coronagraph brightness movie
Synthetic LASCO C3 coronagraph brightness movie
Synthetic LASCO C3 coronagraph running difference movie
Synthetic LASCO C3 coronagraph running difference movie
Synthetic LASCO C3 coronagraph base difference movie
Synthetic LASCO C3 coronagraph base difference movie
Synthetic LASCO C2 coronagraph brightness movie
Synthetic LASCO C2 coronagraph brightness movie
Synthetic LASCO C2 coronagraph running difference movie
Synthetic LASCO C2 coronagraph running difference movie
Synthetic LASCO C2 coronagraph base difference movie
Synthetic LASCO C2 coronagraph base difference movie
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