Alfv\'enic Thermospheric Upwelling in a Global Geospace Model

TL;DR

This study models how Alfvén wave energy deposition causes thermospheric upwelling and density enhancements near the cusp, improving predictions of satellite-observed density variations during geomagnetic activity.

Contribution

It introduces a parameterized Alfvén wave electric field model into the NCAR CMIT model, enhancing thermospheric density predictions during geomagnetic events.

Findings

Inclusion of Alfvénic Joule heating improves density predictions by up to 15%.

The model captures density enhancements near the cusp not predicted by empirical models.

Density changes of 20-30% influence polar region dynamics.

Abstract

Motivated by low-altitude cusp observations of small-scale (~ 1 km) field-aligned currents (SSFACs) interpreted as ionospheric Alfv\'en resonator modes, we investigated the effects of Alfv\'en 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 Alfv\'en 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. CMIT diagnostics for the thermospheric mass density at 400 km altitude show: 1) CMIT without Alfv\'enic Joule heating usually underestimates CHAMP's orbit-average density; inclusion of Alfv\'enic heating modestly improves CMIT's orbit-average prediction of the density (by a few %), especially during the more active periods of the SIR event. 2) The improvement in CMIT's instantaneous density prediction with Alfv\'enic heating included is more significant (up to 15%) in the vicinity of the cusp heating region, a feature that the MSIS empirical thermosphere model misses for this event. Thermospheric density changes of 20-30% caused by the cusp-region Alfv\'enic heating sporadically populate the polar region through the action of corotation and neutral winds.