CMR Header

CCMC Metadata Registry (CMR)

Menu Page

Go to:

 CMR: View Simulation Run Info

PBMOD/6.3/ROR/joseph_olwendo_012225_IT_1

Run Description 

CCMC ROR run for PBMOD 6.3 with RORID joseph_olwendo_012225_IT_1

Simulation Time:

Simulation Start Time: 2025-01-22T08:07:45Z
Simulation End Time: 2025-01-22T08:07:45Z
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 :

joseph.olwendo, 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 Description Caveats Units Default Value or Actual Value Valid Min Valid Max
run_duration 
run duration
 hour 30
utinc 
output_time_interval
 15 min
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 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 
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 
Horizontal Wind Model 2007 (HWM07)
Atmosphere model 
MSIS (Hedin, 1987)
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+ are calculated
from the local model of Jasperse [1974]; production rates
used the solar EUV fluxes derived from the algorithm of
Hinteregger [1981].
ut0 
starting time (UT hours)
 hr 0
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) :

ionospheri scintillation, irregularities

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

spase://CCMC/SimulationModel/PBMOD/6.3

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