Atmosphere Ionosphere Magnetosphere Section - AIM

Global Scale Wave Model (GSWM)

The GSWM solves the linearized and extended Navier-Stokes equations for steady-state global temperature and wind perturbations. GSWM may be used to calculate an "unforced" planetary wave response for a specified period and zonal wavenumber, or the thermally-driven response for either a diurnal or semidiurnal atmospheric tide.

Coupled Magnetosphere Ionosphere Thermosphere Model (CMIT)

The Coupled Magnetosphere Ionosphere Thermosphere (CMIT) model consists of the Lyon-Fedder-Mobarry (LFM) model of the magnetosphere coupled to the Thermosphere-Ionosphere-Electrodynamics General Circulation Model (TIE-GCM).

Assimilative Mapping of Ionospheric Electrodynamics (AMIE)

The AMIE procedure is an optimally constrained, weighted least-squares fit of electric potential distribution to diverse types of atmospheric observations. Knowledge of these distributions is important in many areas of magnetospheric, ionospheric, and thermospheric physics.

Atmosphere-Ionosphere-Magnetosphere

Research Goal

Momentum Budget of the Migrating Diurnal Tide

Friday, November 2, 2012

An analysis was done of the momentum budget of the diurnal westward-propagating wavenumber-1 (DW1) tide simulated by the Whole Atmosphere Community Climate Model (WACCM).

MAGNETOTAIL SCIENCE AND AURORA VIEWING

Aurora Image

HAO Scientist Michael Wiltberger attended the AGU Chapman Conference on Fundamental Properties and Processes of Magnetotails in Reykjavik, Iceland, March 10-15, 2013.

Earth's Magnetosphere

This image is a snapshot from the Lyon-Fedder-Mobarry (LFM) Global Magnetosphere Model. The LFM helps scientists study the interaction between the Sun's magnetic field plasma and the Earth's magnetic field.

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