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SAMI3 (3.20)

SAMI3: Global Ionosphere/Plasmasphere Model

Model Description

SAMI3 (Sami3 is A Model of the Ionosphere) is a seamless, three-dimensional, physics-based model of the ionosphere. It is based on SAMI2, a two-dimensional model of the ionosphere [Huba et al., 2000]. SAMI3 models the plasma and chemical evolution of seven ion species (H+, He+, N+, O+, N+2, NO+ and O+2). The temperature equation is solved for three ion species (H+, He+ and O+) and for the electrons. Ion inertia is included in the ion momentum equation for motion along the geomagnetic field. This is important in modeling the topside ionosphere and plasmasphere where the plasma becomes collisionless. The neutral composition, temperature, and winds can be specified in SAMI3 by the empirical models NRLMSISE00 and HWM14. SAMI3 includes 21 chemical reactions and radiative recombination. SAMI3 uses the EUVAC model for solar radiation. SAMI3 uses a nonorthogonal, nonuniform, fixed grid for the magnetic latitude range +/- 88 degrees. The electric field, driven by the neutral wind dynamo, is determined from the solution of a 2D potential equation [Huba et at., 2008]. The high latitude electric field is calculated from the empirical Weimer model for the potential. The model uses the Richmond apex model [Richmond, 1995] to specify the magnetic field (i.e., IGRF).

Model Figure(s) :

Model Inputs Description

F10.7 (1 day)
F10.7A (3 month average)
Ap index
Kp Index
day-of-year
year

Model Outputs Description

ion density
ion temperature
ion velocity
electron temperature
NmF2
hmF2
TEC (Total Electron Content)
Electron Density
ExB drifts 

Model Caveats


	
	
	
	

Change Log


	
	 
	

Model Acknowledgement/Publication Policy (if any)


	
	
	

Model Domains:

Global_Ionosphere

Space Weather Impacts:

Ionosphere variability (navigation, communications)

Phenomena :

Variablility_of_Plasma_Density
Equatorial_Anomaly
Traveling_Ionospheric_Disturbances

Simulation Type(s):

Physics-based

Temporal Dependence Possible? (whether the code results depend on physical time?)

true

Model is available at?

CCMC

Source code of the model is publicly available?

false

CCMC Model Status (e.g. onboarding, use in production, retired, only hosting output, only source is available):

retired

Code Language:

fortran

Regions (this is automatically mapped based on model domain):

Earth.NearSurface.Ionosphere

Contacts :

Joseph.D.Huba, ModelDeveloper
Min-Yang.Chou, ModelHostContact
Jia.Yue, ModelHostContact
Katherine.Garcia-Sage, ModelHostContact

Acknowledgement/Institution :

Relevant Links :

Publications :

  • Huba, J.D., G. Joyce, and J.A. Fedder, SAMI2 (Sami2 is Another Model of the Ionosphere): A New Low-Latitude Ionosphere Model J. Geophys. Res., 105, 23,035, 2000.
  • Huba, J.D., G. Joyce, and J. Krall, Three-dimensional equatorial spread F modeling, Geo- phys. Res. Lett. 35, L10102, doi:10.1029/2008GL033509, 2008.
  • Richmond, A., Ionospheric electrodynamics using magnetic apex coordinates, J. Geomag. Geoelec. 47, 191, 1995.
  • Huba, J.D. and G. Joyce, Global modeling of equatorial plasma bubbles, Geophys. Res. Lett. 37, L17104, doi:10.1029/2010GL044281, 2010.
  • Huba, J.D. and J. Krall, Modeling the plasmasphere with SAMI3, Geophys. Res. Lett. 40, doi:10.1029/2012GL054300, 2013.
  • Huba, J.D. and H.-L. Liu, Global modeling of equatorial spread F with SAMI3/WACCM-X, Geophys. Res. Lett., 47, e2020GL088258, doi:10.1029/2020GL088258, 2020.
  • Model Access Information :

    Linked to Other Spase Resource(s) (example: another SimulationModel) :

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