HR: 0800h
AN: SA51A-0238 [Abstracts]
TI: Ionospheric Modeling: Coupling to the Inner and Outer Magnetosphere
AU: * Huba, J D
EM: huba@ppd.nrl.navy.mil
AF: Naval Research Laboratory, Code 6790, Washington, DC 20375, United States
AU: Slinker, S
EM: slinker@ppd.nrl.navy.mil
AF: Naval Research Laboratory, Code 6790, Washington, DC 20375, United States
AU: Joyce, G
EM: joyce@ppd.nrl.navy.mil
AF: Icarus Research, Inc., 7113 Exfair Road, Bethesda, MD 20814, United States
AU: Sazykin, S
EM: sazykin@rice.edu
AF: Rice University, 6100 Main St, Houston, TX 77005, United States
AU: Wolf, R
EM: rawolf@rice.edu
AF: Rice University, 6100 Main St, Houston, TX 77005, United States
AU: Spiro, R
EM: spiro@rice.edu
AF: Rice University, 6100 Main St, Houston, TX 77005, United States
AB:
The Naval Research Laboratory has developed a comprehensive
3D model of the earth's ionosphere: SAMI3 (Sami3 is Another
a Model of the Ionosphere).
SAMI3 models the plasma and chemical evolution of seven ion species
(H+, He+, N+, O+, N2+, NO2+ and O2+).
The complete ion
temperature equation is solved for three ion species
(H+, He+ and O+) as well as the electron
temperature equation. Ion inertia is included in the ion momentum
equation for motion along the geomagnetic field. In addition,
the E × B drift motion of the plasma is included for
both zonal electric fields (vertical drifts) and meridional
electric fields (zonal drifts). The neutral species are specified
using the empirical NRLMSISE00 model that is based on MSIS86
and the HWM model. SAMI3 uses a nonorthogonal, nonuniform, fixed grid.
The code has been recently upgraded to provide global
coverage of the ionosphere (± 89° magnetic latitude)
within the context of a single model. The code has been
self-consistently electrodynamically coupled to the
Rice Convection Model (RCM) and to
the Lyon/Fedder/Mobarry (LFM) magnetosphere model.
We report results of ionospheric
dynamics associated with electrodynamic forcing by
the inner and outer magnetosphere, e.g., the convection of
plasma across the polar cap, the impact of
storm-time penetration electric fields on the low- to mid-latitude
ionosphere, and sub-auroral polarization streams. \smallskip
Research supported by ONR and NASA.
DE: 2431 Ionosphere/magnetosphere interactions (2736)
DE: 2443 Midlatitude ionosphere
DE: 2447 Modeling and forecasting
DE: 2475 Polar cap ionosphere
SC: SPA-Aeronomy [SA]
MN: 2007 Fall Meeting