Linking Solar Minimum, Space Weather, and Night Sky Brightness

Abstract New observations indicate previously unrecognized significant sources of night sky brightness variations, not involving corresponding changes in the Sun's EUV flux , occur during deep solar minimum. Our data was taken at 5 sites spanning more than 8,500 km during the deep minimum of Solar Cycle 24 into the beginning of Solar Cycle 25. It shows; 1) Semi-annual night sky brightness variations are produced by interactions between the Earth's magnetic field and the interplanetary magnetic field. 2) Solar wind plasma streams from solar coronal holes produce major night sky brightness increase events. 3) Some night sky brightness events are relatively local. Others extend at least 8,500 km along the Earth's surface. 4) It is plausible, terrestrial night airglow and geomagnetic indices have similar responses to the solar energy input into Earth's magnetosphere. Our empirical results contribute to a quantitative basis for understanding and predicting night sky brightness variations. They are applicable in astronomical, space weather, light pollution, biological, and recreational studies.