Dayglow emissions below 200 km on Mars show minimal differences between crustal and non-crustal magnetic field regions on the dayside, with larger variations near the terminator and across seasons.
The Astrophysical Journal Letters, 853(2), p.L33
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Investigation of Martian UV Dayglow Emissions in the Southern Hemisphere during Solar Quiet-time Conditions: Insights from Multi-year MAVEN/IUVS Observations
Dayglow emissions below 200 km on Mars show minimal differences between crustal and non-crustal magnetic field regions on the dayside, with larger variations near the terminator and across seasons.