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ENLIL/2.8f/ROR/emiliya_yordanova_110821_SH_1

Run Description

CCMC ROR run for ENLIL 2.8f with RORID emiliya_yordanova_110821_SH_1

Simulation Time:

Simulation Start Time: 2020-07-14T00:00:00Z
Simulation End Time: 2021-11-08T19:51:04Z
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 :

michelle.mendoza, 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
stationary_Solar_Wind
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. GNG
CRot
Carrington Rotation number
2233
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)
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 0 90
cloud_velocity
Cloud velocity for each of the specified clouds
km/s 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
spherical
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) :

gong2233

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

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

List of Publications Referencing this Run :

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Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Collection Consent Agreement