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ENLIL/2.8f/ROR/Marianna_Felici_090522_SH_2

Run Description 

CCMC ROR run for ENLIL 2.8f with RORID Marianna_Felici_090522_SH_2

Simulation Time:

Simulation Start Time: 2017-10-09T00:00:00Z
Simulation End Time: 2017-10-09T00:00:00Z
Time Step in second:
Simulation Time Description:
Simulation Time Caveats:

Temporal Dependence (whether the outputs of the simulation code are time-dependent?): true

Regions:

Heliosphere.Inner

Simulation Domain :

Contacts :

Marianna.Felici, ModelUser

List of Run Input Parameter Grouping and their associated properties :

Name Description Caveats Properties
Settings for the model 
Settings used to run the model
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
run_subtype 
Physical nature of the run - to generate a stationary solar wind solution or to run ENLIL with the cone model
 cone_model
inner_boundary 
Source of the inner boundary
 from_WSA_model
initial_state 
Source of the initial state
 analytic_prescription
outer_boundary 
The last planet included within the outer Radial Boundary.
Mars
observatory 
Magnetogram Source
 If interested in several magnetogram sources, please submit separate runs, one for each magnetogram source. We do provide runs using GONG data. However please be aware that the GONG data is still being used in trial mode and there are some known issues with the polar fields which are currently being studied by the GONG staff. NSO
CRot 
Carrington Rotation number
 2196
Grid 
Grid
 256x30x90
fast_solar_wind_density 
Density of the fast Solar Wind for the cone model
 The ENLIL model assumes that the wind speed at the models inner radial boundary is both supersonic and super-alfvenic. The default parameters for the 'fast wind' are set to ensure that this is true for almost all magnetograms. If you choose to vary the fast wind properties, bear in mind that this may cause these conditions to be violated. cm-3 300
fast_solar_wind_temperature 
Temperature of the fast Solar Wind for the cone model
 The ENLIL model assumes that the wind speed at the models inner radial boundary is both supersonic and super-alfvenic. The default parameters for the 'fast wind' are set to ensure that this is true for almost all magnetograms. If you choose to vary the fast wind properties, bear in mind that this may cause these conditions to be violated. million Kelvin (MK) 0.8
fast_solar_wind_velocity 
Speed of the fast Solar Wind for the cone model
 The ENLIL model assumes that the wind speed at the models inner radial boundary is both supersonic and super-alfvenic. The default parameters for the 'fast wind' are set to ensure that this is true for almost all magnetograms. If you choose to vary the fast wind properties, bear in mind that this may cause these conditions to be violated. km/s 625
number_of_clouds 
Number of CME clouds to insert
 1
clouds_start_dates 
Start date of each of the specified clouds (date YYYY-MM-DD when cloud center at inner boundary)
 2017-10-10T00:08
cloud_latitude 
Latitude of cloud center for each of the specified clouds (north=90, equator=0, south=-90 degs)
 HEEQ 0 -90 90
cloud_longitude 
Longitude of cloud center for each of the specified clouds (Range: -180 to 180 degs, where 0 degrees is earthward)
 HEEQ 0 -180 180
cloud_radius 
Radius (half-width)for each of the specified clouds
 deg 25 0 90
cloud_velocity 
Cloud velocity for each of the specified clouds
 km/s 650 250 3000
density_enhancement 
Density enhancement factor for each of the specified clouds (cloud density over fast stream value)
 4 1 10
temperature_enhancement 
Temperature enhancement factor for each of the specified clouds (cloud temperature over fast stream value)
 1 0.5 10
elongation_factor 
Elongation factor of the trailing part of the cloud  for each of the specified clouds (1 for sphere, 2 for twice longer and so on up to 5)
 1 1 5
cloud_shape 
Shape of the cloud for each of the specified clouds
 2
cloud_cavity_radius 
Cloud cavity radius over cloud radius value for each of the specified clouds
 0 0 0.9

Run Access Information :

Keyword(s) :

Mars_aurora

Linked to Parent Spase Resource(s) (example: SimulationModel) :

spase://CCMC/SimulationModel/ENLIL/2.8f

List of Publications Referencing this Run :

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