Thermospheric density perturbations produced by Traveling Atmospheric Disturbances during August 2005 storm

The MAGE simulation, which resolved mesoscale high-latitude convection electric fields and field-aligned currents, and included physics-based specification of auroral precipitation, was contrasted with a standalone ionosphere-thermosphere simulation driven by a high-latitude electrodynamics empirical model. The comparison demonstrates that first-principles representations of highly dynamic and localized Joule heating events in a fully coupled whole geospace model is critical to accurately capture both generation and propagation of traveling atmospheric disturbances (TADs) that produce neutral density perturbations globally.

The MAGE simulation shows that larger density peaks in the equatorial region observed by CHAMP and GRACE are the result of TADs generated at high-latitudes in both hemispheres, and intersect at low-latitudes. This study reveals the importance of investigating thermospheric density variations at all latitudes in a fully coupled geospace model with sufficiently high resolving power.