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PBMOD/6.3/ROR/Andres_CardenasContreras_060923_IT_5

Run Description 

CCMC ROR run for PBMOD 6.3 with RORID Andres_CardenasContreras_060923_IT_5

Simulation Time:

Simulation Start Time: 2023-06-09T16:13:52Z
Simulation End Time: 2023-06-09T16:13:52Z
Time Step in second: 15 min
Simulation Time Description:
Simulation Time Caveats:

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

Regions:

Earth.NearSurface.Ionosphere

Simulation Domain :

Contacts :

Andres.Cardenas, ModelUser

List of Run Input Parameter Grouping and their associated properties :

Name Description Caveats Properties
All settings for PBMOD model 
All settings for PBMOD model
Name Label Description Caveats Units Default Value or Actual Value Valid Min Valid Max
run_duration run_duration 
run duration
 hour 7
utinc utinc 
output_time_interval
 15 min
f10.7 f10.7 
F10.7 - solar radio flux at 10.7 cm - used as a measure of solar activity. The model automatically loads the F10.7 values for that day from GFZ
 sfu
Ap Ap 
Ap index - The Ap index is a daily measure of magnetic activity. The model automatically loads the Ap values for that day (https://kp.gfz-potsdam.de/app/files/Kp_ap_Ap_SN_F107_since_1932.txt)
Kp Kp 
Geomagnetic Activity index. The model automatically loads the Kp values for that day. (https://kp.gfz-potsdam.de/app/files/Kp_ap_Ap_SN_F107_since_1932.txt)
Neutral wind model Neutral wind model 
Horizontal Wind Model 2007 (HWM07)
Atmosphere model Atmosphere model 
MSIS (Hedin, 1987)
Ion and electron temperatures Ion and electron temperatures 
The ion and electron temperatures are based on the empirical model of Brace and Theis [1981].
Production and loss rates of O+ Production and loss rates of O+ 
Production and loss rates of O+ are calculated
from the local model of Jasperse [1974]; production rates
used the solar EUV fluxes derived from the algorithm of
Hinteregger [1981].
ut0 ut0 
starting time (UT hours)
 hr 0
lgmdb lgmdb 
Use IGRF field model (+lgmdb). If this is turned off, then the tilted dipole field model is used. (Several of the neutral models do have this turned off for efficiency, -lgmdb, to prevent the gm database from being loaded, since geomagnetic parameters are not used in those models.)

Run Access Information :

Keyword(s) :

\\r\\nIonosphere, Model, GNSS\\r\\n

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

spase://CCMC/SimulationModel/PBMOD/6.3

List of Publications Referencing this Run :

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