Abstract The Solar Occultation (SO) channel of the Nadir and Occultation for Mars Discovery
(NOMAD) instrument scans the Martian atmosphere since 21 April 2018. In this work, we …

Current models underestimate the highest observed ozone (O3) column densities on Mars.
These estimates could be improved by including the uptake of odd hydrogen species (HOx) …

Abstract Haberle et al.(2019) documented the status of the NASA Ames Legacy Mars Global
Climate Model (GCM) and presented a baseline water cycle simulation. Since publishing …

Migrating tides dominate the tropical climate on Mars and are known to reach high
amplitudes during global dust events (GDE). In this study, we characterize the amplitude …

Temperature profiles retrieved using the first set of data of the Emirates Mars InfraRed
Spectrometer obtained during the science phase of the Emirates Mars Mission are used for …

Multilanders and rovers on Mars have observed the diurnal variation in surface pressure
with two significant peaks at dawn and twilight (around 8: 00 am and 8: 00 pm) at different …

Thermal tides are atmospheric planetary‐scale waves with periods that are harmonics of the
solar day. In the Martian atmosphere thermal tides are known to be especially significant …

Boundary-layer winds near steeply sloped topography excite a distinct type of atmospheric
wave. Basic properties of the waves were determined through analysis of 7 Mars years of …

Much of the variability in the Martian thermosphere can be attributed to vertically
propagating atmospheric tides that are known to achieve significant amplitudes in this …

Abstract In early 2019, the Mars Atmosphere and Volatile Evolution (MAVEN) mission
underwent an∼ 2‐month aerobraking campaign during which time the spacecraft periapsis …