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CTIPe (3.2)

Coupled Thermosphere Ionosphere Plasmasphere Electrodynamics Model

Model Description

The Coupled Thermosphere Ionosphere Plasmasphere Electrodynamics Model (CTIPe) model consists of four distinct components:

-A global thermosphere model;
-A high-latitude ionosphere model;
-A mid and low-latitude ionosphere/plasmasphere model;
-An electrodynamical calculation of the global dynamo electric field.

All four components of the CTIPe are run concurrently and are fully coupled with respect to energy, momentum, and continuity.

The thermospheric code simulates the time-dependent global structure of the wind vector, temperature, and density of the neutral thermosphere by numerically solving the non-linear primitive equations of momentum, energy, and continuity on a 3D spherical polar grid rotating with the Earth. The latitude resolution is 2 deg, longitude resolution is 18 deg, and the vertical direction is divided into 15 levels in logarithm of pressure from lower boundary of 1 Pa at 80 km altitude. The equation of motion includes Coriolis effects, horizontal pressure gradients, horizontal and vertical viscosity, and ion drag. The non-linear energy equation describes horizontal and vertical advection of energy, horizontal and vertical heat conduction by both molecular and turbulent diffusion, heating by solar UV and EUV radiation, cooling by infrared radiation, and ionospheric Joule heating. The continuity equation incorporates three major species: atomic oxygen, molecular nitrogen and molecular oxygen and include chemistry, transport and the mutual diffusion between species.

The high-latitude ionosphere convection model calculates field-aligned ion velocity components from the field-aligned momentum equation. The model includes chemistry, gravity, and ion-ion and ion-neutral collisional drag. The ionosphere is computed self-consistently with the thermosphere pole-ward of 23 degrees latitude in both hemispheres. Transport under the influence of magnetospheric electric fields is explicitly treated, assuming ExB drifts and collisions with neutral particles.

The plasmasphere model solves coupled equations of continuity, momentum and energy balance along many closed flux tubes concurrently. The orientation of flux tubes is determined by eccentric dipole approximation to the Earth's magnetic field. Each flux-tube is subject to ExB drift.

Model Figure(s) :

Model Inputs Description


	
	
	
	

Model Outputs Description


	
	
	
	

Model Caveats


	
	
	
	

Change Log


	
	 
	

Model Acknowledgement/Publication Policy (if any)


	
	
	

Model Domains:

Global_Ionosphere
Thermosphere

Space Weather Impacts:

Ionosphere variability (navigation, communications)
Atmosphere variability (satellite/debris drag)

Phenomena :

Variablility_of_Plasma_Density
Atmosphere_Expansion
Neutral_Composition_Change
Neutral_Wind_Change
Ion_Drift_Velocity
Equatorial_Anomaly
Traveling_Ionospheric_Disturbances
Traveling_Atmospheric_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
Earth.NearSurface.Thermosphere

Contacts :

Yuta.Hozumi, ModelHostContact
Tim.Fuller-Rowell, ModelContact
Mihail.Codrescu, ModelContact
Jia.Yue, ModelHostContact
Katherine.Garcia-Sage, ModelHostContact

Acknowledgement/Institution :

NOAA SEC

Relevant Links :

Publications :

Model Access Information :

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

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