Alfvénic thermospheric upwelling in a global geospace model

Motivated by low-altitude cusp observations of small-scale (similar to 1 km) field-aligned currents (SSFACs) interpreted as ionospheric Alfven resonator modes, we have investigated the effects of Alfven wave energy deposition on thermospheric upwelling and the formation of air density enhancements in and near the cusp. Such density enhancements were commonly observed near 400 km altitude by the CHAMP satellite. They are not predicted by empirical thermosphere models, and they are well correlated with the observed SSFACs.

A parameterized model for the altitude dependence of the Alfven wave electric field, constrained by CHAMP data, has been developed and embedded in the Joule heating module of the National Center for Atmospheric Research (NCAR) Coupled Magnetosphere-Ionosphere-Thermosphere (CMIT) model. The CMIT model was then used to simulate the geospace response to an interplanetary stream interaction region (SIR) that swept past Earth on 26-27 March 2003.