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.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
physics.space-ph 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.