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OpenGGCM/4.0/ROR/Yaireska_Collado-Vega_072414_1a

Run Description 

CCMC ROR run for OpenGGCM 4.0 with RORID Yaireska_Collado-Vega_072414_1a

Simulation Time:

Simulation Start Time: 2001-03-24T05:00:00Z
Simulation End Time: 2001-03-24T06:00:00Z
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.Magnetosphere

Simulation Domain :

Contacts :

Yaireska.Collado-Vega, 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
RCM 
Inner magnetosphere model options (with RCM or without RCM / CRCM)
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).
 True
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)
 5 3 9
setting_option_for_Bx 
Indicates how solar wind Bx is set:

Set Bx to a specified constant ('user')
Set Bx to the initial solar wind data value ('init')
Use average Bx from solar wind data ('auto')
 user
b_abs 
Magnitude of IMF
 9.82
b_angle 
IMF clock angle
 -179.59
sw_link 
Solar wind link
 plot
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
 5.43
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
 Yaireska_Collado-Vega_072414_1a_sw.gif
dipole_update 
Flag indicating whether dipole updates throughout the run (True) or dipole set to start time of run (False)
 True
dipole_time 
Dipole time
 2001/03/24 05:00
dipole_tilt 
Dipole tilt
 deg -9.72493
dipole_tilt_y 
Y component of dipole tilt
 deg 23.0696
corotation 
Flag indicating whether to enable corotation around fixed dipole orientation
 real
Run_Ring_Current_Model_or_Not 
Flag indicating whether to run Ring Current Model
Calculate_Oval_Position_or_Not 
Flag indicating whether to run field line tracer to calculate polar cap (region with open field lines).
withRCM 
Flag indicating whether to use RCM inner magnetosphere model
withCIMI 
Flag indicating whether to use CIMI inner magnetosphere model
withCRCM 
Flag indicating whether to use CRCM inner magnetosphere model
withRBE 
Flag indicating whether to use RBE radiation belt model
Provide_Output_Along_Satellite_Trajectory 
Flag indicating whether to generate output files along the trajectory of the tracked satellites
Provide_CDF_Output_files 
Flag indicating whether to provide CDF output files
Provide_HDF_Output_files 
Flag indicating whether to generate HDF output files
Provide_MAGNETOMETER_Output_Files 
Flag indicating whether to generate magnetometer output files
run_type 
Type of the run - either driven by real data or by artificial conditions
 Driven by data
Solar wind inputs 
Time-dependent solar wind plasma and magnetic field inputs.
 Solar wind inputs are derived from a single spacecraft usually 200 R_E upstream of the sun-ward (front) simulation box boundary.
Name Description Caveats Units Default Value or Actual Value Valid Min Valid Max
solarwind 
Flag indicating whether solar wind data are constant (initial values) or variable (var).
 var const var
sw_source 
Name of the spacecraft or data source used to generate solar wind input information. Currently one of ACE-RT ACE-L2, WIND, OMNI, DSCOVR (real time)
 User-submitted data may be from any source or made-up. ACE-L2
constant-Bx 
Constant Bx value fed into the front boundary of the simulation.
 nT 0
By-coefficient 
Coefficient for By in linear combination approximating Bx: Bx ~ constant-Bx + By-coefficient*By + Bz-coefficient*Bz
 0 -1 1
Bz-coefficient 
Coefficient for Bz in linear combination approximating Bx: Bx ~ constant-Bx + By-coefficient*By + Bz-coefficient*Bz
 0 -1 1
Bx 
Sun-Earth component of solar wind magnetic field.
 Bx is usually held constant (zero or average of observed values) to conserve div.B at the front boundary. Alternatively, oblique phase fronts can be assumed that update solar wind conditions along those fronts throughout the front boundary. Bx is then approximated as a linear combination of time dependent By and Bz. nT 0 -100 100
By 
Dawn-dusk component of solar wind magnetic field.
 nT -0.071 -100 100
Bz 
North-south component of the solar wind magnetic field. B_z is most important magnetic field component to drive or inhibit geomagnetic activity. Other components play a role in connection with the orientation of the Earth's dipole field.
 nT -9.816 -100 100
Vx 
Sun-Earth component of solar wind velocity.
 Low solar wind speed (less than 200 km/s in magnitude) usually indicates poor statistics in the solar wind plasma measurements. km/s -438.856 -3000 -200
Vy 
Plasma velocity in dawn-dusk direction.
 The orbital velocity of Earth (about 29 km/s) is usually neglected. km/s 14.182 -500 500
Vz 
Solar wind plasma velocity in north-south direction.
 km/s -9.816 -500 500
N 
Solar wind plasma density.
 Mass density described in terms of number of protons per cubic centimeter. AMU/cm^3 8.924 0.1 100
T 
Solar wind plasma temperature.
 Derived from observed distribution of solar wind particles. Can fluctuate widely when density N is at or below 1 AMU/cm^3. K 100076 10000 2000000
SW density floor 
Lowest value of N applied during pre-processing of solar wind input data.
 The density floor in the solar wind varies by magnetosphere model and it's numerical stability. A similar floor may be imposed inside the magnetotail lobes where the density may drop lower than in the solar wind. AMU/cm^3 2.5 0.1 2.5
Ionosphere conductance model 

						
						
						
												 
						
							

								
									

										Name
										Description
										Caveats
										Units
										Default Value or Actual Value
										Valid Min
										Valid Max
									

								
								
								
								

									iono_conductance
									
Parameter indicationg selection of conductance model in the ionosphere electrodynamics component of the model.

									The two models offered for run-on-request are constant (user sets Pedersen Conductance and Hall Conductance) and auroral (conducances driven by f10.7 and field-aligned currents from magnetosphere part of the model).
									
									auroral
									constant
									auroral
									
								

								
								

									Pedersen Conductance
									
Value of constant user-selected Pedersen Conductance in the ionosphere.

									
									S
									
									1
									100
									
								

								
								

									Hall Conductance
									
Value of constant user-selected Hall Conductance in the ionosphere.

									
									S
									
									0
									100
									
								

								
								

									f10.7
									
Solar irradiation index as represented by the flux of 10.7 cm (2800 MHz) radiation from the Sun measured in units of 10−22 W⋅m−2⋅Hz−1.

									Daily index of solar radiation that affects the daytime background conductivity in the ionosphere.
									sfu
									217.5
									50
									300
									
								

								
								
							

						
						
						
					

				
					

						Magnetosphere model parameters
						

						
						
						
												 
						
							

								
									

										Name
										Description
										Caveats
										Units
										Default Value or Actual Value
										Valid Min
										Valid Max
									

								
								
								
								

									inflow boundary
									
Location of sun-ward facing (front) boundary of the magnetosphere simulation box.

									
									R_E
									-33
									24
									128
									
								

								
								

									grid
									
Magnetosphere grid

									
									
									
									
									
									
								

								
								
							

						
						
						
					

				
					

						Model outputs
						
Parameters that define the type of outputs generated and the frequency of outputs.

						
						
						
												 
						
							

								
									

										Name
										Description
										Caveats
										Units
										Default Value or Actual Value
										Valid Min
										Valid Max
									

								
								
								
								

									SSCWeb_satellite_names
									
Comma-separated list of satellite names (single-word strings used in SSCweb).

									Satellite trajectories are obtained from SSCweb's Locator Tabular interface and are typically limited to missions in geospace.
									
									chandra,cluster1,cluster2,cluster3,cluster4,geotail,goes10,goes11,goes8,goes9,image,imp8,lanl89,lanl90,lanl91,lanl94,lanl97,moon,polar,wind
									
									all satellites in SSCweb that are aloft at any time during a model run's time interval
									
								

								
								

									satellite_output_time_interval
									
Time interval between outputs during satellite tracking in the magnetosphere (or inner mangetosphere) model.

									
									s
									5
									1
									60
									
								

								
								

									satellite_names
									
Comma-separated list of satellite names

									Satellite trajectories are obtained from SSCweb's Locator Tabular interface and are typically limited to missions in geospace.
									
									Chandra,Cluster-1 (FM5/Rumba),Cluster-2 (FM6/Salsa),Cluster-3 (FM7/Samba),Cluster-4 (FM8/Tango),Geotail,GOES-10,GOES-11,GOES-8,GOES-9,IMAGE,IMP-8,LANL-89,LANL-90,LANL-91,LANL-94,LANL-97,Moon,Polar,Wind
									
									all satellites in SSCweb that are aloft at any time during a model run's time interval
									
								

								
								
							

						
						
						
					

				
			
		

	

	

		Run Access Information
		
		:
	

	
	
	

		Keyword(s)
		
		:
	

	
		
			Magnetopause Crossing

		
	
	
	

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

	
	
		
							
				
					spase://CCMC/SimulationModel/OpenGGCM/4.0

				
				
				
						
		
	
	
	
	

		List of Publications Referencing this Run  
		
		:
	

	
	


        		
    

    

        
            




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