The high latitude ionospheric evolution of the May 10-11, 2024, geomagnetic storm is investigated in terms of Total Electron Content and contextualized with Incoherent Scatter Radar and ionosonde observations. Substantial plasma lifting is observed within the initial Storm Enhanced Density plume with ionospheric peak heights increasing by 150km to 300km, reaching levels of up to 630km. Scintillation is observed within the cusp during the initial expansion phase of the storm, spreading across the auroral oval thereafter. Patch transport into the polar cap produces broad regions of scintillation that are rapidly cleared from the region after a strong Interplanetary Magnetic Field reversal at 2230UT. Strong heating and composition changes result in the complete absence of the F2-layer on the 11th, suffocating high latitude convection from dense plasma necessary for Tongue of Ionization and patch formation, ultimately resulting in a suppression of polar cap scintillation on the 11th.

The Mid-latitude All-sky-imaging Network for Geophysical Observations (MANGO) employs a combination of two powerful optical techniques used to observe the dynamics of Earth’s upper atmosphere: wide-field imaging and high-resolution spectral interferometry. Both techniques observe the naturally occurring airglow emissions produced in the upper atmosphere at 630.0- and 557.7-nm wavelengths. Instruments are deployed to sites across the continental United States, providing the capability to make measurements spanning mid to sub-auroral latitudes. The current instrument suite in MANGO has five all-sky imagers observing the 630.0-nm emission (integrated between ~250-400 km altitude), four all-sky imagers observing the 557.7-nm emission (integrated between ~97-100 km altitude), and three Fabry-Perot interferometers measuring neutral winds and temperature using both these wavelengths. The deployment of additional imagers is planned. The network makes unprecedented observations of the nighttime thermosphere-ionosphere dynamics with the expanded field-of-view provided by the distributed network of instruments. This paper describes the network, the instruments, the data products, and first results from this effort.