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Ovation-Prime/2.3/ROR/SaiGowtam_Valluri_021524_IT_6

Run Description 

CCMC ROR run for Ovation-Prime 2.3 with RORID SaiGowtam_Valluri_021524_IT_6

Simulation Time:

Simulation Start Time: 2013-06-01T00:00:00Z
Simulation End Time: 2013-06-30T23:59:00Z
Time Step in second: 60
Simulation Time Description:
Simulation Time Caveats:

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

Regions:

Earth.NearSurface.Ionosphere.Topside

Simulation Domain :

Contacts :

SaiGowtam.Valluri, ModelUser

List of Run Input Parameter Grouping and their associated properties :

Name Description Caveats Properties
All settings for Ovation Prime model 
All settings used to run Ovation Prime model
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
solarwind 
Property indicating whether solar wind is a fixed value ('fixed') or varies ('var', i.e., uploaded as a file or obtained from a data set).
 var
sw_source 
Property indicating source of solar wind data
 OMNI
despike_solar_wind_data 
Flag indicating whether to automatically de-spike solar wind (optional for automatically retrieved data only; use when solar wind data shown in next page have clusters of extreme values in plasma density, temperature or velocity).
 False
despike.threshold 
De-spike threshold (standard deviations)
 sigmas 3 2 4
despike.number_of_samples 
De-spike length (number of samples in cluster of extreme values to be eliminated)
 7 3 9
b_abs 
Magnitude of IMF
 9.62
b_angle 
IMF clock angle
 -66.3
Bx 
Bx component of IMF (Interplanetary Magnetic Field). IMF is a geomagnetic index used in external magnetic field model computation. It corresponds to the part of the Sun's magnetic field that is carried into interplanetary space by the solar wind. The three orthogonal components of the IMF are Bx, By and Bz. Bx and By are oriented parallel to the ecliptic. The IMF is a weak field, varying in strength near the Earth from 1 to 37 nT, with an average value of about 6 nT.
 nT -4.103
By 
By component of IMF (Interplanetary Magnetic Field). IMF is a geomagnetic index used in external magnetic field model computation. It corresponds to the part of the Sun's magnetic field that is carried into interplanetary space by the solar wind. The three orthogonal components of the IMF are Bx, By and Bz. Bx and By are oriented parallel to the ecliptic. The IMF is a weak field, varying in strength near the Earth from 1 to 37 nT, with an average value of about 6 nT.
 nT -8.809
Bz 
Bx component of IMF (Interplanetary Magnetic Field). IMF is a geomagnetic index used in external magnetic field model computation. It corresponds to the part of the Sun's magnetic field that is carried into interplanetary space by the solar wind. The three orthogonal components of the IMF are Bx, By and Bz. Bx and By are oriented parallel to the ecliptic. The IMF is a weak field, varying in strength near the Earth from 1 to 37 nT, with an average value of about 6 nT.
 nT 3.866
Vx 
X component of plasma velocity
 km/s -399.228
Vy 
Y component of plasma velocity
 km/s -28.037
Vz 
Z component of plasma velocity
 km/s -14.579
den 
Plasma density
 cm-3
temp 
Plasma temperature
 K
use_AP_from_archive 
Flag indicating whether to use observed AP index from archive or calculate AP index from solar wind inputs
 False
AP_index_value 
Value of AP index
 0
sw_link 
Solar wind link
 plot
SW_density_floor 
Solar wind density floor value
SW_density_floor_was_applied 
Flag indicating the solar wind density has been floored with SW_density_floor value to ensure that the model will run through the requested time interval.
 False
minimum_SW_Fast-Mode_mach_number 
Minimum solar wind Fast-Mode mach number
 1.33
SW_parameters_are_large 
Flag indicating whether solar wind velocity, density or dynamic pressure are large. If they are, the run is a special request requiring attention by CCMC staff. The variables will be accepted unless they exceed certain absolute maximum values.
SW_plot 
Name of solar wind plot
 SaiGowtam_Valluri_021524_IT_6_sw.gif
dipole_update 
True: Dipole Orientation is Consistent with the Real Time During The Simulated Time Interval. Dipole Orientation is Updated With Time. False: Dipole Orientation is Fixed to a select dipole tilt (-34 deg < tilt < 34 deg).
 The Earth's dipole tilt is used as an input to Weimer model to calculate ionospheric potential used by CTIP. True
dipole_time 
Dipole time
 2013/06/01 00:00
dipole_tilt 
Dipole tilt
 deg 19.6157
dipole_tilt_y 
Y component of dipole tilt
 deg 17.9821
inflow_boundary 
Upstream inflow boundary
 0

Run Access Information :

Keyword(s) :

precipitation

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

spase://CCMC/SimulationModel/Ovation-Prime/2.3

List of Publications Referencing this Run :

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