Measuring Mars Atmospheric Winds from Orbit

@article{Baker2020MeasuringMA,
  title={Measuring Mars Atmospheric Winds from Orbit},
  author={S. A. Baker and J. Battalio and T. Bertrand and A. Brown and A. Colaprete and A. Cook and D. Cremons and M. Crismani and A. Dave and M. Day and M. Desjean and M. Elrod and L. Fenton and J. Fisher and L. Gordley and P. Hayne and N. Heavens and J. Hollingsworth and D. Jha and V. Jha and M. Kahre and A. Khayat and A. Kling and S. Lewis and B. T. Marshall and G. Mart'inez and L. Montabone and M. Mischna and C. Newman and A. Pankine and H. Riris and J. Shirley and M. D. Smith and A. Spiga and X. Sun and L. Tamppari and R. Young and D. Vi'udez-Moreiras and G. Villaneuva and M. Wolff and R. Wilson},
  journal={arXiv: Instrumentation and Methods for Astrophysics},
  year={2020}
}
Wind is the process that connects Mars' climate system. Measurements of Mars atmospheric winds from orbit would dramatically advance our understanding of Mars and help prepare for human exploration of the Red Planet. Multiple instrument candidates are in development and will be ready for flight in the next decade. We urge the Decadal Survey to make these measurements a priority for 2023-2032. 

References

SHOWING 1-10 OF 64 REFERENCES
Planet-wide sand motion on Mars
Prior to Mars Reconnaissance Orbiter data, images of Mars showed no direct evidence for dune and ripple motion. This was consistent with climate models and lander measurements indicating that windsExpand
Global circulation of Mars’ upper atmosphere
TLDR
Mapping of the global circulation in the thermosphere of Mars with the Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft reveals circulation patterns simpler than those of Earth that persist over changing seasons. Expand
First Absolute Wind Measurements in the Middle Atmosphere of Mars
The first absolute wind measurements in the middle atmosphere of Mars (40-70 km) were obtained from Doppler shifts in the J = 1-2 CO transition at 230.538 GHz. During the 1988 opposition, this lineExpand
Design of a direct-detection wind and aerosol lidar for mars orbit
The present knowledge of the Mars atmosphere is greatly limited by a lack of global measurements of winds and aerosols. Hence, measurements of height-resolved wind and aerosol profiles are a priorityExpand
Vertical temperature profile and mesospheric winds retrieval on Mars from CO millimeter observations Comparison with general circulation model predictions
Aims. We have recorded high spectral resolution spectra and derived precise atmospheric temperature profiles and wind velocities in the atmosphere of Mars. We have compared observations of theExpand
Wind measurements in Mars' middle atmosphere: IRAM Plateau de Bure interferometric CO observations
The IRAM Plateau de Bure Interferometer has been used to map the CO(1–0) rotational line in Mars' middle atmosphere. Absolute winds and thermal profiles were retrieved during the 1999, 2001, 2003 andExpand
Mars Climate Sounder limb profile retrieval of atmospheric temperature, pressure, and dust and water ice opacity
The Mars Climate Sounder (MCS) onboard the Mars Reconnaissance Orbiter is the latest of a series of investigations devoted to improving the understanding of current Martian climate. MCS is aExpand
Thermal Tides in the Martian Middle Atmosphere as Seen by the Mars Climate Sounder.
TLDR
Using a Martian General Circulation Model to extend the analysis, it is shown that the diurnal thermal tide dominates these patterns for all latitudes and all seasons. Expand
Long term wind erosion on Mars
Abstract Wind erosion and deposition are powerful agents of surface change on Mars. Erosion is sensitive to the atmospheric density, so feedback between orbit variations and atmospheric density canExpand
Stormy water on Mars: The distribution and saturation of atmospheric water during the dusty season
TLDR
Water profiles during the 2018–2019 southern spring and summer stormy seasons show that high-altitude water is preferentially supplied close to perihelion, and supersaturation occurs even when clouds are present, implying that the potential for water to escape from Mars is higher than previously thought. Expand
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