Mineralogy, composition, and alteration of Mars Pathfinder rocks and soils: Evidence from multispectral, elemental, and magnetic data on terrestrial analogue, SNC …

RV Morris, DC Golden, JF Bell III… - Journal of …, 2000 - Wiley Online Library
Major element, multispectral, and magnetic properties data were obtained at Ares Vallis
during the Mars Pathfinder mission. To understand the compositional, mineralogical, and …

Mineralogic and compositional properties of Martian soil and dust: Results from Mars Pathfinder

JF Bell III, HY McSween Jr, JA Crisp… - Journal of …, 2000 - Wiley Online Library
Mars Pathfinder obtained multispectral, elemental, magnetic, and physical measurements of
soil and dust at the Sagan Memorial Station during the course of its 83 sol mission. We …

Image simulation and assessment of the colour and spatial capabilities of the Colour and Stereo Surface Imaging System (CaSSIS) on the ExoMars Trace Gas Orbiter

LL Tornabene, FP Seelos, A Pommerol… - Space Science …, 2018 - Springer
This study aims to assess the spatial and visible/near-infrared (VNIR) colour/spectral
capabilities of the 4-band Colour and Stereo Surface Imaging System (CaSSIS) aboard the …

Regional dust deposits on Mars: Physical properties, age, and history

PR Christensen - Journal of Geophysical Research: Solid Earth, 1986 - Wiley Online Library
Major dust storms on Mars play an important role in the deposition and removal of fine dust
material. Thermal, radar, and visual remote sensing observations provide important …

Viking Lander image analysis of Martian atmospheric dust

JB Pollack, ME Ockert‐Bell… - Journal of Geophysical …, 1995 - Wiley Online Library
We have reanalyzed three sets of Viking Lander 1 and 2 (VL1 and VL2) images of the
Martian atmosphere to better evaluate the radiative properties of the atmospheric dust …

Results from the Mars Pathfinder camera

PH Smith, JF Bell III, NT Bridges, DT Britt, L Gaddis… - Science, 1997 - science.org
Images of the martian surface returned by the Imager for Mars Pathfinder (IMP) show a
complex surface of ridges and troughs covered by rocks that have been transported and …

[HTML][HTML] The zodiacal light from 1.0 to 0.3 AU as observed by the Helios space probes

C Leinert, I Richter, E Pitz… - … , vol. 103, no. 1, Nov. 1981 …, 1981 - adsabs.harvard.edu
The average properties of zodiacal light are summarized as obtained from several years of
observations from the Helios 1 and 2 space probes. Consistent results on intensity, color …

Absorption and scattering properties of the Martian dust in the solar wavelengths

ME Ockert‐Bell, JF Bell III, JB Pollack… - Journal of …, 1997 - Wiley Online Library
A new wavelength‐dependent model of the single‐scattering properties of the Martian dust
is presented. The model encompasses the solar wavelengths (0.3 to 4.3 μm at 0.02 μm …

Mars surface composition from reflectance spectroscopy: A summary

RB Singer, TB McCord, RN Clark… - Journal of …, 1979 - Wiley Online Library
Visible and near‐infrared (0.3–2.6 μm) reflectance spectra of the martian surface have been
obtained primarily from earth‐based telescopic observations, and multispectral images have …

Spectral evidence for the mineralogy of high‐albedo soils and dust on Mars

RB Singer - Journal of Geophysical Research: Solid Earth, 1982 - Wiley Online Library
Because of the lack of direct mineralogic data available for Mars, spectral remote sensing
techniques and, in particular, earth‐based reflectance spectroscopy remain the primary …