In the near future, much of the Earth's lightning activity will be continuously monitored from space by lightning imagers placed in geostationary orbit. These new satellite-based instruments open a new era of weather monitoring and research into the role of thunderstorm processes in the dynamics of the atmosphere and in climate change. The Geostationary Lightning Mapper (GLM) on the first of the Geostationary Operational Environmental Satellite GOES-R Series (GOES-16 at 75.2 W) is the first lightning detector in geostationary orbit (Goodman et al., 2013; Rudlosky et al., 2019a, 2019b). GLM is based on its predecessors, the Optical Transient Detector (OTD) and Lightning Imaging Sensor (LIS) Boccippio et al., 2002, Christian et al., 1989). In China, the Lightning Mapping Imager (LMI) on the Feng-Yun4 is detecting lightning in Asia (Yang et al., 2017) and in the near future, Europe and Africa will be continuously monitored by the Lightning Imager (LI) on the Meteosat Third Generation satellites (MTG) (Stuhlmann et al., 2005). All of these systems, new to the geostationary orbit, use optical imagers at the narrow spectral line at the 777.4 nm infrared emission of atomic oxygen that is associated with hot lightning channels (e.g., Soler et al., 2020). The Atmosphere-Space Interactions Monitor (ASIM) on the International Space Station (ISS) consists of a suite of optical instruments and X-ray and gamma-ray detectors for investigating lightning, Transient Luminous Events (TLEs) and Terrestrial Gamma-ray Flashes (TGFs) (e.g., Chanrion et al., 2019; Neubert et al., 2019). ASIM is equipped with three photometers at 180-230 nm, 337.0 and 777.4 nm spectral bands plus two one-megapixel cameras at 337.0 and 777.4 nm. The objective of the 337.0 nm (blue) and 777.4 nm