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Pressure observations by the Curiosity rover: Initial results

TLDR
In this paper, the pressure measurement subsystem of the Mars Science Laboratory (MSL) Rover Environmental Measurement Station (REMS-P) performed accurate observations of the Martian atmospheric surface pressure.
Abstract
[1] REMS-P, the pressure measurement subsystem of the Mars Science Laboratory (MSL) Rover Environmental Measurement Station (REMS), is performing accurate observations of the Martian atmospheric surface pressure. It has demonstrated high data quality and good temporal coverage, carrying out the first in situ pressure observations in the Martian equatorial regions. We describe the REMS-P initial results by MSL mission sol 100 including the instrument performance and data quality and illustrate some initial interpretations of the observed features. The observations show both expected and new phenomena at various spatial and temporal scales, e.g., the gradually increasing pressure due to the advancing Martian season signals from the diurnal tides as well as various local atmospheric phenomena and thermal vortices. Among the unexpected new phenomena discovered in the pressure data are a small regular pressure drop at every sol and pressure oscillations occurring in the early evening. We look forward to continued high-quality observations by REMS-P, extending the data set to reveal characteristics of seasonal variations and improved insights into regional and local phenomena.

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The atmosphere of Mars as observed by InSight

Don Banfield, +63 more
- 24 Feb 2020 - 
TL;DR: The InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander is measuring Mars's atmosphere with unprecedented continuity, accuracy and sampling frequency.
References
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Journal ArticleDOI

Improved general circulation models of the Martian atmosphere from the surface to above 80 km

TL;DR: In this paper, a set of two general circulation models of the Martian atmosphere derived from the models originally developed in the early 1990s are described. But the models share the same physical parameterizations but use two complementary numerical methods to solve the atmospheric dynamic equations.
Journal ArticleDOI

The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment

TL;DR: The Mars Pathfinder atmospheric structure investigation/meteorology (ASI/MET) experiment measured the vertical density, pressure, and temperature structure of the martian atmosphere from the surface to 160 km, and monitored surface meteorology and climate for 83 sols.
Journal ArticleDOI

Mars atmospheric dynamics as simulated by the NASA Ames General Circulation Model: 1. The zonal-mean circulation

TL;DR: In this article, the characteristics of the zonal-mean circulation and how it responds to seasonal variations and dust loading are described, and the radiative effects of suspended dust particles, even in small amounts, have a major influence on the general circulation.
Journal ArticleDOI

Meteorological results from the surface of Mars: Viking 1 and 2

TL;DR: The meteorology equipment carried by the Viking landers was intended to measure atmospheric temperature, wind speed, wind direction, and pressure as discussed by the authors, with a complex hodograph and the Lander-1 site, dominated by counterclockwise turning of the wind, and a simpler hoderograph at the lander-2 site, marked by clockwise turning the wind.
Journal ArticleDOI

Occultation Experiment: Results of the First Direct Measurement of Mars's Atmosphere and Ionosphere

TL;DR: Preliminary analysis of changes in the frequency, phase, and amplitude of the Mariner IV radio signal, caused by passage through the atmosphere and ionosphere of Mars, have yielded estimates of the refractivity and density of the atmosphere near the surface, the scale height in the atmosphere, and the electron density profile of the Martian ionosphere.
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