CMR Header

CCMC Metadata Registry (CMR)

Menu Page

Go to:

 CMR: View Simulation Run Info

TIE-GCM/2.5/ROR/Dipjyoti_Patgiri_010424_IT_10

Run Description 

CCMC ROR run for TIE-GCM 2.5 with RORID Dipjyoti_Patgiri_010424_IT_10

Simulation Time:

Simulation Start Time: 2021-06-19T00:20:00Z
Simulation End Time: 2021-07-19T00:20:00Z
Time Step in second: 1200
Simulation Time Description:
Simulation Time Caveats:

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

Regions:

Earth.NearSurface.Atmosphere
Earth.NearSurface.Ionosphere
Earth.NearSurface.Thermosphere

Simulation Domain :

Contacts :

DIPJYOTI.PATGIRI, 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
E_field_model 
E_field_model
 WEIMER
resolution 
resolution
 default
Kp 
Geomagnetic Activity index. If KP is specified and POWER and/or CTPOTEN are commented, then the given KP will be used with empirical formulas to calculate POWER and/or CTPOTEN, which are used in the Auroral parameterization.

KP can be provided as a scalar constant (KP), or as a series of time-dependent values (KP_TIME), as in the below examples. KP cannot be set if GPI_NCFILE data file is specified.

Empirical formula used to calculate POWER from KP (see function hp_from_kp in util.F):

if (kp <=7.) hp_from_kp = 16.82*exp(0.32*kp)-4.86
if (kp > 7.) hp_from_kp = 153.13 + (kp-7.)/(9.-7.)*(300.-153.13)
Empirical formula used to calculate CTPOTEN from KP (see function ctpoten_from_kp in util.F):

ctpoten_from_kp = 15.+15.*kp + 0.8*kp**2

Examples:
KP = 4.0
KP_TIME = 80,0,0,4., 80,6,0,4.5, 80,12,0,5.0
 0 0 9
SWden 
Solar Wind Density (#/cm-3). Can be specified as either a constant (SWDEN), or series of time-dependent values (SWDEN_TIME). If IMF_NCFILE is set and SWDEN is not provided, then it SWDEN will be taken from the IMF data file.

Data type: real or real array

Examples:
SWDEN = 4.0 ; constant for entire run
SWDEN_TIME = 80,0,0,2., 80,1,0,3., 80,2,0,4. ; time series
#/cm-3
SWvel 
Solar Wind Velocity (Km/s). Can be specified as either a constant (SWVEL), or series of time-dependent values (SWVEL_TIME). If IMF_NCFILE is set and SWVEL is not provided, then it SWVEL will be taken from the IMF data file.

Data type: real or real array

Examples:
SWVEL = 400. ; constant for entire run
SWVEL_TIME = 80,0,0,100., 80,1,0,200., 80,2,0,300. ; time series
 Km/s
ztop 
Upper model boundary height. Examples: ZTOP =7, the model upper boundary is around 500 km at solar max. ZTOP = 11, the upper boundary is around 1000 km at solar max.
 9
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
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 -100 100
By 
Dawn-dusk component of solar wind magnetic field.
 nT -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 -100 100
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
									0
									50
									300
									
								

								
								
							

						
						
						
					

				
			
		

	

	

		Run Access Information
		
		:
	

	
	
	

		Keyword(s)
		
		:
	

	
		
			Meridional and zonal wind, O/N2 Ratio

		
	
	
	

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

	
	
		
							
				
					spase://CCMC/SimulationModel/TIE-GCM/2.5

				
				
				
						
		
	
	
	
	

		List of Publications Referencing this Run  
		
		:
	

	
	


        		
    

    

        
            




CMR Footer





 



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