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Assimilative Mapping of Electron Flux Using SSUSI Lyman-Birge-Hopfield Emissions
Far ultraviolet (FUV) imaging of the aurora from space provides great insight into the dynamic coupling of the Earth’s atmosphere, ionosphere and magnetosphere on global scales. To gain quantitative understanding of these coupling processes, the global distribution of auroral energy flux is required, but the inversion of FUV emission to derive precipitating auroral particles’ energy flux is not straightforward. Furthermore, the spatial coverage of FUV imaging from LEO altitudes is often insufficient to achieve global map ...
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Assimilative mapping; Electron flux; Far ultraviolet imaging; Lyman-Birge-Hopfield emission