| 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 |
|
|
2088 |
|
|
| Grid |
Grid |
|
|
1024x120x360 |
|
|
| 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 |
CCMC Metadata Registry (CMR)