Atmospheric Imaging Results from the Mars Exploration Rovers: Spirit and Opportunity

@article{Lemmon2004AtmosphericIR,
  title={Atmospheric Imaging Results from the Mars Exploration Rovers: Spirit and Opportunity},
  author={Mark T. Lemmon and Michael J. Wolff and M. D. Smith and Robert T. Clancy and D Banfield and Geoffrey A. Landis and A. Ghosh and P. H. Smith and Nicole Spanovich and Barbara Anne Whitney and Patrick L. Whelley and Ronald Greeley and Shane D. Thompson and J F Bell and Steven W. Squyres},
  journal={Science},
  year={2004},
  volume={306},
  pages={1753 - 1756}
}
A visible atmospheric optical depth of 0.9 was measured by the Spirit rover at Gusev crater and by the Opportunity rover at Meridiani Planum. Optical depth decreased by about 0.6 to 0.7% per sol through both 90-sol primary missions. The vertical distribution of atmospheric dust at Gusev crater was consistent with uniform mixing, with a measured scale height of 11.56 ± 0.62 kilometers. The dust's cross section weighted mean radius was 1.47 ± 0.21 micrometers (μm) at Gusev and 1.52 ± 0.18 μ at… 
Measuring Nighttime Atmospheric Opacity Using Images From the Mars Exploration Rovers
Measuring Nighttime Atmospheric Opacity Using Images From the Mars Exploration Rovers. (April 2010) Keri Marie Bean Department of Atmospheric Sciences Texas A&M University Research Advisor: Dr. Mark
Mapping Martian Atmospheric Pressure with Ground-Based Near Infrared Spectroscopy
Abstract We present images of Mars obtained in the 2.0 μm CO2 band with the United Kingdom Infrared Telescope (UKIRT). The images reveal topographic features of the Martian surface that are usually
Optical depth and its scale-height in Valles Marineris from HRSC stereo images
One Martian year of atmospheric observations using MER Mini‐TES
[1] The Spirit and Opportunity Mars Exploration Rovers (MER) landed on the surface of Mars in January 2004. Thermal infrared spectra taken by the Miniature Thermal Emission Spectrometer (Mini-TES)
Spectrophotometric properties of materials observed by Pancam on the Mars Exploration Rovers: 2. Opportunity
[1] The Panoramic Camera (Pancam) on the Mars Exploration Rover Opportunity acquired visible/near-infrared multispectral observations of soils and rocks under varying viewing and illumination
Surface scattering properties at the Opportunity Mars rover's traverse region measured by CRISM
The Opportunity Rover has been exploring Meridiani Planum; concurrently, the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) has been collecting orbital hyperspectral data. Herein, both
...
1
2
3
4
5
...

References

SHOWING 1-10 OF 30 REFERENCES
Properties of dust in the Martian atmosphere from the Imager on Mars Pathfinder
The Imager for Mars Pathfinder (IMP) returned sequences of images of the Martian sky characterizing the size distribution, optical constants, and nature of the aerosols suspended in the atmosphere of
Opacity of the Martian atmosphere measured by the Imager for Mars Pathfinder
The Imager for Mars Pathfinder (IMP) has obtained 1733 images of the Sun during its 83-sol mission starting on July 4, 1997, which have been used to determine the atmospheric opacity at wavelengths
First Atmospheric Science Results from the Mars Exploration Rovers Mini-TES
Thermal infrared spectra of the martian atmosphere taken by the Miniature Thermal Emission Spectrometer (Mini-TES) were used to determine the atmospheric temperatures in the planetary boundary layer
Optical properties of the Martian aerosols as derived from Imager for Mars Pathfinder midday sky brightness data
The Imager for Mars Pathfinder (IMP) obtained data on the midday sky brightness in filters centered at 443.6, 481.0, 670.8, 896.1 and 965.3 nm. Useful data sets were returned on sols 27, 40, 56, 65,
Localization and Physical Property Experiments Conducted by Opportunity at Meridiani Planum
TLDR
The low mechanical strength of the evaporitic rocks as determined from grinding experiments, and the abundance of coarse-grained surface particles argue for differential erosion of Meridiani Planum.
Localization and Physical Properties Experiments Conducted by Spirit at Gusev Crater
TLDR
Physical properties experiments show a decrease of 0.2% per Mars solar day in solar cell output resulting from deposition of airborne dust, cohesive soil-like deposits in plains and hollows, bright and dark rock coatings, and relatively weak volcanic rocks of basaltic composition.
Pancam Multispectral Imaging Results from the Spirit Rover at Gusev Crater
Panoramic Camera images at Gusev crater reveal a rock-strewn surface interspersed with high- to moderate-albedo fine-grained deposits occurring in part as drifts or in small circular swales or
Miniature Thermal Emission Spectrometer for the Mars Exploration Rovers
[1] The Miniature Thermal Emission Spectrometer (Mini-TES) will provide remote measurements of mineralogy and thermophysical properties of the scene surrounding the Mars Exploration Rovers and guide
...
1
2
3
...