Since the inception of mass spectrometry more than a century ago, the field has matured as
analytical capabilities have progressed, instrument configurations multiplied, and …

The Martian surface environment today is cold and dry, but evidence suggests the planet
may have hosted more habitable conditions in the past. Open questions about the evolution …

Mars dayside thermospheric temperature and scale height trends were examined using
measurements from the Neutral Gas Ion Mass Spectrometer (NGIMS) and the Imaging …

Lower atmospheric global dust storms affect the small‐and large‐scale weather and
variability of the whole Martian atmosphere. Analysis of the CO2 density data from the …

Wavelike perturbations in the Martian upper thermosphere observed by the Neutral Gas Ion
Mass Spectrometer (NGIMS) onboard the Mars Atmosphere and Volatile EvolutioN …

The Mars thermosphere (above approximately 120 km) has been probed in situ for one Mars
year using accelerometers on board the Mars Atmosphere and Volatile Evolution (MAVEN) …

The paper presents observations of gravity wave‐induced temperature disturbances in the
Martian atmosphere obtained with the mid‐infrared (MIR) spectrometer, a channel of the …

The burst of Mars exploration in the past two decades has significantly improved our
knowledge of the Martian atmosphere. A variety of complementary, multiannual …

Gravity waves (GWs) are important for vertical coupling between the lower and upper
atmosphere on Mars. Saturated GWs will promote the acceleration of mean flow and …

We present an analysis of gravity waves in Mars' upper atmosphere above 120 km. Using in-
situ data from NGIMS onboard MAVEN we have been able to characterise waves from …