Welcome to MANGO
The Midlatitude Allsky-imaging Network for GeoSpace Observations (MANGO) is a collection of cameras spread across the continental United States with the goal of imaging large-scale airglow and aurora features. MANGO will be used to observe the generation, propagation, and dissipation of medium and large-scale wave activity in the subauroral, mid and low-latitude thermosphere. This network is actively being deployed and will ultimately consist of nine all-sky imagers. These imagers form a network providing continuous coverage over the western United States, including California, Oregon, Washington, Utah, Arizona and Texas extending south into Mexico. This network sees high levels of both medium and large scale wave activity.