SubAuroral Red Arc Generated by Inner Magnetosphere Heat Flux

CIMI_HF_fig1.nc contains processed energetic H+ and O+ ion energy spectra measured by the HOPE instrument onboard RBSP-B satellite, and electron heat flux derived from the RBSP data and simulated by the Comprehensive Inner Magnetosphere Ionosphere model. CIMI_HF_fig2.nc contains electron temperature, density, and red line 6300 A emission rate from the TIEGCM simulation experiment for CIMI heat flux.

CIMI_HF_fig3a.nc contains the zonal ion drift from the empirical SAPS model.CIMI_HF_fig3b.nc contains electron temperature, density, and red line 6300 A emission rate from the TIEGCM simulation experiment for empirical SAPS. CIMI_HF_fig4a.nc contains the 6300 A emission rate from the baseline and CIMI heat flux TIEGCM runs.CIMI_HF_fig4b.nc contains the 6300 A emission rate from the baseline and empirical SAPS TIEGCM runs.