Solar Control of the Martian Dayglow: A Decade of MAVEN/IUVS Observations

fits_data.txt-- MAVEN/IUVS L1 c limb observations for CO Cameron, CO2+ UVD and OI 297.2 nm emissions, between 18 October 2014 to and 14 May 2025.
cameron_peak_info.csv--Chapman fitting results (peak intensity, peak altitude, and corresponding geometric parameters), for the limb profile of CO Cameron bands.
uvd_peak_info.csv--Chapman fitting results (peak intensity, peak altitude, and corresponding geometric parameters), for the limb profile of CO2+ UVD.
o2972_peak_info.csv--Chapman fitting results (double-peak intensity, double-peak altitude, and corresponding geometric parameters), for the limb profile of OI 297.2 nm emission.
cameron_solar_flux.csv--The simultaneous solar X-ray and EUV flux at Mars relates to the CO Cameron limb measurements.
uvd_solar_flux.csv--The simultaneous solar X-ray and EUV flux at Mars relates to the CO2+ UVD limb measurements.
o2972_solar_flux.csv--The simultaneous solar X-ray and EUV flux at Mars relates to the OI 297.2 nm limb measurements.
cameron_sf_H.csv-- Scale height derived from the CO Cameron emission varies with the corresponding solar X-ray and EUV flux.
uvd_sf_H.csv-- Scale height derived from the CO2+ UVD emission varies with the corresponding solar X-ray and EUV flux.
o2972_sf_H.csv-- Scale height derived from the OI 297.2 nm emission varies with the corresponding solar X-ray and EUV flux.
cameron_ls_H.csv-- Scale height derived from the CO Cameron emission varies with the corresponding solar longitude.
uvd_ls_H.csv-- Scale height derived from the CO2+ UVD emission varies with the corresponding solar longitude.
o2972_ls_H.csv-- Scale height derived from the OI 297.2 nm emission varies with the corresponding solar longitude.