Joule heating and radiative cooling usually play key roles in high-latitude thermospheric temperature changes during geomagnetic storms. In the mesosphere and lower thermosphere (MLT), however, the causes of storm-time temperature changes at high latitudes are still elusive. Here, we elucidate the nature and mechanisms of MLT temperature variations at high latitudes during the 10^th September 2005 storm by diagnostically analyzing the MLT thermodynamics in the Thermosphere Ionosphere Mesosphere Electrodynamics General Circulation Model (TIMEGCM) simulations. In the storm’s initial and main phases, the MLT temperature decreases at 0:00 Local Time (LT) -12:00 LT, but increases in the 12:00 LT-24:00 LT sector at high latitudes. Afterward, the temperature decrease disappears and temperature increase occurs at all local times in the high latitudes. Adiabatic heating/cooling and vertical advection associated with vertical winds are the main drivers of high-latitude temperature changes in the entire altitude range of the MLT region. However, around the auroral oval and above ~100 km, the Joule heating rate is comparable to the heating caused by vertical advection and adiabatic heating/cooling associated with vertical winds and becomes one of the major contributors to total heating in the high-latitude MLT region. The effects of Joule heating can penetrate down to ~95 km. Horizontal advection also plays a key role in storm-time MLT temperature changes inside the polar cap and becomes larger than the adiabatic heating/cooling above ~105 km.

MLT,地磁暴,中性温度