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