Investigations of exothermic heating and OH nightglow variations induced by a gravity wave packet at 18 degree south

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[0310] Atmospheric Composition And Structure / Airglow And Aurora, [0340] Atmospheric Composition And Structure / Middle Atmosphere: Composition And Chemistry, [0341] Atmospheric Composition And Structure / Middle Atmosphere: Constituent Transport And Chemistry, [0342] Atmospheric Composition And Structure / Middle Atmosphere: Energy Deposition

Scientific paper

This study aims to examine wave-induced secular variations of exothermic heating and OH nightglow in the MLT region with a 2D OH chemistry-dynamics model. The model is capable of simulating the time evolution of the minor species reacting in the OH nightglow in the wakes of a gravity wave packet. The wave packet is simulated with a spectral full wave model. Previous studies show that the OH nightglow variations are latitudinal-dependent. In this study, we will examine the variations of OH nightglow and the associated exothermic heating at latitude 18 degrees south and compare the results to the previous studies at the same latitude but in the northern hemisphere to gain a better understanding if there is any hemispheric difference.

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