Investigation of Martian UV Dayglow Emissions in the Southern Hemisphere during Solar Quiet-time Conditions: Insights from Multi-year MAVEN/IUVS Observations

This study presents a comprehensive analysis of prominent ultraviolet (UV) dayglow emissions in the southern hemisphere of Mars under solar quiet-time conditions, utilizing five Martian years (MY 33–37) of data from the MAVEN/IUVS instrument. It investigates the potential influence of crustal magnetic fields on these emissions across different seasons, as well as in both the dayside and dayside-terminator regions.