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Tsyganenko/TS05/ROR/Karen_Ferreira_040224_IM_1

Run Description 

CCMC ROR run for Tsyganenko TS05 with RORID Karen_Ferreira_040224_IM_1

Simulation Time:

Simulation Start Time: 2013-10-02T01:00:00Z
Simulation End Time: 2013-10-02T02:00:00Z
Time Step in second: 240
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 :

Karen.Ferreira, 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
KP_type 
Type of Kp data (definite or provisional or realtime or user-uploaded)
 provisional
type_of_F107_data 
Type of F10.7 data (Kp_3h or corrected_fluxdata)
 NOAA/Kp_3h
b_abs 
Magnitude of IMF
 3.96
b_angle 
IMF clock angle
 -167.02
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
 2.44
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
 Karen_Ferreira_040224_IM_1_sw.gif
dipole_time 
Dipole time
 2013/10/02 01:00
dipole_tilt 
Dipole tilt
 deg -9.45378
dipole_tilt_y 
Y component of dipole tilt
 deg -15.1063
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. OMNI-1min
constant-Bx 
Constant Bx value fed into the front boundary of the simulation.
 nT 3.4
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 3.4 -100 100
By 
Dawn-dusk component of solar wind magnetic field.
 nT -0.89 -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 -3.86 -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 -364.8 -3000 -200
Vy 
Plasma velocity in dawn-dusk direction.
 The orbital velocity of Earth (about 29 km/s) is usually neglected. km/s 41.717 -500 500
Vz 
Solar wind plasma velocity in north-south direction.
 km/s -25.037 -500 500
N 
Solar wind plasma density.
 Mass density described in terms of number of protons per cubic centimeter. AMU/cm^3 1.55 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 125597 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 0.01 0.1 2.5
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
									10
									24
									128
									
								

								
								
							

						
						
						
					

				
					

						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
									

								
								
								
								

									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.
									
									RBSP-A,RBSP-B,THEMIS-A (P5),THEMIS-D (P3),THEMIS-E (P4)
									
									all satellites in SSCweb that are aloft at any time during a model run's time interval
									
								

								
								

									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.
									
									rbspa,rbspb,themisa,themisd,themise
									
									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
									240
									1
									60
									
								

								
								
							

						
						
						
					

				
					

						Ionosphere conductance model
						

						
						
						
												 
						
							

								
									

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

								
								
								
								

									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
									108.30
									50
									300
									
								

								
								
							

						
						
						
					

				
			
		

	

	

		Run Access Information
		
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		Keyword(s)
		
		:
	

	
		
			pre ICME

		
	
	
	

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

	
	
		
							
				
					spase://CCMC/SimulationModel/Tsyganenko Magnetic Field/TS05

				
				
				
						
		
	
	
	
	

		List of Publications Referencing this Run  
		
		:
	

	
	


        		
    

    

        
            




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