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Moore CA, Moores JE, Newman CE, Lemmon MT, Guzewich SD, Battalio M. Vertical and Horizontal Heterogeneity of Atmospheric Dust Loading in Northern Gale Crater, Mars. ICARUS 2019; 329:197-206. [PMID: 31359883 PMCID: PMC6662233 DOI: 10.1016/j.icarus.2019.03.041] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/10/2023]
Abstract
This paper updates the record of atmospheric dust loading within northern Gale Crater, Mars, by providing line-of-sight extinction (LOS-Ext) measurements of the intervening dust between the rover and the crater rim. These measurements are derived from images taken with the Navigation Cameras (Navcam) onboard the Mars Science Laboratory (MSL) rover, Curiosity. The observations span 2.44 Mars years, from Mars Year (MY) 31 at a solar longitude (L S ) of 208° to t L S = 7° of MY34, sols 100 - 1701 of the MSL surface mission. This work examines the dataset for seasonal trends of the LOS-Ext in addition to horizontal variations and the vertical structure of LOS-Ext. The LOS-Ext has a repetitive pattern with a single peak in the latter half of the Mars year. The atmosphere in the crater is well mixed horizontally but not vertically as larger LOS-Ext is seen nearer the crater floor than at higher altitudes within the crater. The results allow a discussion on whether or not Gale Crater is a sink for atmospheric dust or a source of atmospheric dust in the current era.
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Affiliation(s)
- Casey A Moore
- York University, Centre for Research in Earth and Space Sciences (CRESS), 4700 Keele Street, Toronto ON M3J 1P3, Canada
| | - John E Moores
- York University, Centre for Research in Earth and Space Sciences (CRESS), 4700 Keele Street, Toronto ON M3J 1P3, Canada
| | | | - Mark T Lemmon
- Texas A&M University, Department of Atmospheric Sciences, MS 3150 College Station, Texas 77843, United States
| | - Scott D Guzewich
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, United States
| | - Michael Battalio
- Texas A&M University, Department of Atmospheric Sciences, MS 3150 College Station, Texas 77843, United States
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2
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Liu W, Chen S, Wu CY, Li S. Unified size-density and size-topology relations in random packings of dry adhesive polydisperse spheres. Phys Rev E 2019; 99:022901. [PMID: 30934263 DOI: 10.1103/physreve.99.022901] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/08/2018] [Indexed: 11/07/2022]
Abstract
We study the size-density and size-topology relations in random packings of dry adhesive polydisperse microspheres with Gaussian and lognormal size distributions through a geometric tessellation. We find that the dependence of the neighbor number on the centric particle size is always quasilinear, regardless of the size distribution, size span, or interparticle adhesion. The average local packing fraction as a function of normalized particle size for different size variances is well regressed on the same profile, which increases to larger values as the relative strength of adhesion decreases. The variations of the local coordination number with the particle size converge onto a single curve for all adhesive particles, but gradually transfer to another branch for nonadhesive particles. Such adhesion-induced size-density and size-topology relations are interpreted theoretically with a modified geometrical "granocentric" model, where the model parameters are dependent on a single dimensionless adhesion number. Our findings, together with the modified theory, provide a more unified perspective on the substantial geometry of amorphous polydisperse systems, especially those with fairly loose structures.
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Affiliation(s)
- Wenwei Liu
- Department of Chemical and Process Engineering, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - Sheng Chen
- Key Laboratory for Thermal Science and Power Engineering of Ministry of Education, Department of Energy and Power Engineering, Tsinghua University, Beijing 100084, China
| | - Chuan-Yu Wu
- Department of Chemical and Process Engineering, University of Surrey, Guildford GU2 7XH, United Kingdom
| | - Shuiqing Li
- Key Laboratory for Thermal Science and Power Engineering of Ministry of Education, Department of Energy and Power Engineering, Tsinghua University, Beijing 100084, China
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3
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Seasonal Deposition and Lifting of Dust on Mars as Observed by the Curiosity Rover. Sci Rep 2018; 8:17576. [PMID: 30514860 PMCID: PMC6279765 DOI: 10.1038/s41598-018-35946-8] [Citation(s) in RCA: 24] [Impact Index Per Article: 4.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/13/2018] [Accepted: 11/12/2018] [Indexed: 11/08/2022] Open
Abstract
In situ measurements by the Curiosity rover provide a unique opportunity for studying the effects of dust on assets placed at the surface of Mars. Here we use in situ measurements of solar UV radiation to quantify the seasonal and interannual variability of dust accumulation on the sensor on the rover deck. We show that the amount of dust accumulated on the sensor follows a seasonal cycle, with net dust removal during the perihelion season until Ls ~ 300°, and net dust deposition until the end of the aphelion season (Ls ~ 300°-180°). We use independent in situ measurements of atmospheric opacity and pressure perturbations in combination with numerical modeling, showing that daytime convective vortices and nighttime winds are likely responsible for the seasonal dust cleaning, with the role of nighttime wind being more important in Martian Year (MY) 32 than in MY 33 and that of daytime convective vortices being more important in MY 33 than in MY 32. The fact that the UV sensor is cleaner in MY 33 than in MY 32 indicates that natural cleaning events make solar energy an excellent candidate to power extended (multiannual) Mars missions at similar latitudes as the Curiosity rover.
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Bridges JC, Clemmet J, Croon M, Sims MR, Pullan D, Muller JP, Tao Y, Xiong S, Putri AR, Parker T, Turner SMR, Pillinger JM. Identification of the Beagle 2 lander on Mars. ROYAL SOCIETY OPEN SCIENCE 2017; 4:170785. [PMID: 29134081 PMCID: PMC5666264 DOI: 10.1098/rsos.170785] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 06/27/2017] [Accepted: 09/13/2017] [Indexed: 06/07/2023]
Abstract
The 2003 Beagle 2 Mars lander has been identified in Isidis Planitia at 90.43° E, 11.53° N, close to the predicted target of 90.50° E, 11.53° N. Beagle 2 was an exobiology lander designed to look for isotopic and compositional signs of life on Mars, as part of the European Space Agency Mars Express (MEX) mission. The 2004 recalculation of the original landing ellipse from a 3-sigma major axis from 174 km to 57 km, and the acquisition of Mars Reconnaissance Orbiter High Resolution Imaging Science Experiment (HiRISE) imagery at 30 cm per pixel across the target region, led to the initial identification of the lander in 2014. Following this, more HiRISE images, giving a total of 15, including red and blue-green colours, were obtained over the area of interest and searched, which allowed sub-pixel imaging using super high-resolution techniques. The size (approx. 1.5 m), distinctive multilobed shape, high reflectivity relative to the local terrain, specular reflections, and location close to the centre of the planned landing ellipse led to the identification of the Beagle 2 lander. The shape of the imaged lander, although to some extent masked by the specular reflections in the various images, is consistent with deployment of the lander lid and then some or all solar panels. Failure to fully deploy the panels-which may have been caused by damage during landing-would have prohibited communication between the lander and MEX and commencement of science operations. This implies that the main part of the entry, descent and landing sequence, the ejection from MEX, atmospheric entry and parachute deployment, and landing worked as planned with perhaps only the final full panel deployment failing.
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Affiliation(s)
- J. C. Bridges
- Leicester Institute for Space and Earth Observation, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
| | - J. Clemmet
- Airbus, Gunnels Wood Road, Stevenage SG1 2AS, UK
| | | | - M. R. Sims
- Leicester Institute for Space and Earth Observation, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
| | - D. Pullan
- Leicester Institute for Space and Earth Observation, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
| | - J.-P. Muller
- Mullard Space Science Laboratory, Department of Space and Climate Physics, University College London, Holmbury St Mary RH5 6NT, UK
| | - Y. Tao
- Mullard Space Science Laboratory, Department of Space and Climate Physics, University College London, Holmbury St Mary RH5 6NT, UK
| | - S. Xiong
- Mullard Space Science Laboratory, Department of Space and Climate Physics, University College London, Holmbury St Mary RH5 6NT, UK
| | - A. R. Putri
- Mullard Space Science Laboratory, Department of Space and Climate Physics, University College London, Holmbury St Mary RH5 6NT, UK
| | - T. Parker
- Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA
| | - S. M. R. Turner
- Leicester Institute for Space and Earth Observation, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
| | - J. M. Pillinger
- School of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK
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Abstract
The scientific objectives of the ExoMars rover are designed to answer several key questions in the search for life on Mars. In particular, the unique subsurface drill will address some of these, such as the possible existence and stability of subsurface organics. PanCam will establish the surface geological and morphological context for the mission, working in collaboration with other context instruments. Here, we describe the PanCam scientific objectives in geology, atmospheric science, and 3-D vision. We discuss the design of PanCam, which includes a stereo pair of Wide Angle Cameras (WACs), each of which has an 11-position filter wheel and a High Resolution Camera (HRC) for high-resolution investigations of rock texture at a distance. The cameras and electronics are housed in an optical bench that provides the mechanical interface to the rover mast and a planetary protection barrier. The electronic interface is via the PanCam Interface Unit (PIU), and power conditioning is via a DC-DC converter. PanCam also includes a calibration target mounted on the rover deck for radiometric calibration, fiducial markers for geometric calibration, and a rover inspection mirror. Key Words: Mars—ExoMars—Instrumentation—Geology—Atmosphere—Exobiology—Context. Astrobiology 17, 511–541.
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Liu W, Chen S, Li S. Influence of adhesion on random loose packings of binary microparticle mixtures. AIChE J 2017. [DOI: 10.1002/aic.15775] [Citation(s) in RCA: 11] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
Affiliation(s)
- Wenwei Liu
- Dept. of Thermal Engineering, Key Laboratory for Thermal Science and Power Engineering of Ministry of Education; Tsinghua University; Beijing 100084 China
| | - Sheng Chen
- Dept. of Thermal Engineering, Key Laboratory for Thermal Science and Power Engineering of Ministry of Education; Tsinghua University; Beijing 100084 China
| | - Shuiqing Li
- Dept. of Thermal Engineering, Key Laboratory for Thermal Science and Power Engineering of Ministry of Education; Tsinghua University; Beijing 100084 China
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Korablev OI, Dobrolensky Y, Evdokimova N, Fedorova AA, Kuzmin RO, Mantsevich SN, Cloutis EA, Carter J, Poulet F, Flahaut J, Griffiths A, Gunn M, Schmitz N, Martín-Torres J, Zorzano MP, Rodionov DS, Vago JL, Stepanov AV, Titov AY, Vyazovetsky NA, Trokhimovskiy AY, Sapgir AG, Kalinnikov YK, Ivanov YS, Shapkin AA, Ivanov AY. Infrared Spectrometer for ExoMars: A Mast-Mounted Instrument for the Rover. ASTROBIOLOGY 2017; 17:542-564. [PMID: 28731817 DOI: 10.1089/ast.2016.1543] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/07/2023]
Abstract
ISEM (Infrared Spectrometer for ExoMars) is a pencil-beam infrared spectrometer that will measure reflected solar radiation in the near infrared range for context assessment of the surface mineralogy in the vicinity of the ExoMars rover. The instrument will be accommodated on the mast of the rover and will be operated together with the panoramic camera (PanCam), high-resolution camera (HRC). ISEM will study the mineralogical and petrographic composition of the martian surface in the vicinity of the rover, and in combination with the other remote sensing instruments, it will aid in the selection of potential targets for close-up investigations and drilling sites. Of particular scientific interest are water-bearing minerals, such as phyllosilicates, sulfates, carbonates, and minerals indicative of astrobiological potential, such as borates, nitrates, and ammonium-bearing minerals. The instrument has an ∼1° field of view and covers the spectral range between 1.15 and 3.30 μm with a spectral resolution varying from 3.3 nm at 1.15 μm to 28 nm at 3.30 μm. The ISEM optical head is mounted on the mast, and its electronics box is located inside the rover's body. The spectrometer uses an acousto-optic tunable filter and a Peltier-cooled InAs detector. The mass of ISEM is 1.74 kg, including the electronics and harness. The science objectives of the experiment, the instrument design, and operational scenarios are described. Key Words: ExoMars-ISEM-Mars-Surface-Mineralogy-Spectroscopy-AOTF-Infrared. Astrobiology 17, 542-564.
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Affiliation(s)
| | | | | | | | - Ruslan O Kuzmin
- 1 Space Research Institute IKI , Moscow, Russia
- 2 Vernadsky Institute of Geochemistry and Analytical Chemistry GEOKHI , Moscow, Russia
| | - Sergei N Mantsevich
- 1 Space Research Institute IKI , Moscow, Russia
- 3 Department of Physics, Lomonosov Moscow State University , Russia
| | | | - John Carter
- 5 Institut d'Astrophysique Spatiale IAS-CNRS/Université Paris Sud , Orsay, France
| | - Francois Poulet
- 5 Institut d'Astrophysique Spatiale IAS-CNRS/Université Paris Sud , Orsay, France
| | - Jessica Flahaut
- 6 Université Lyon 1 , ENS-Lyon, CNRS, UMR 5276 LGL-TPE, Villeurbanne, France
| | - Andrew Griffiths
- 7 Mullard Space Science Laboratory, University College London , Dorking, United Kingdom
| | - Matthew Gunn
- 8 Department of Physics, Aberystwyth University , Aberystwyth, United Kingdom
| | | | - Javier Martín-Torres
- 10 Division of Space Technology, Department of Computer Science, Electrical and Space Engineering, Luleå University of Technology , Kiruna, Sweden
- 11 Instituto Andaluz de Ciencias de la Tierra (CSIC-UGR) , Granada, Spain
| | - Maria-Paz Zorzano
- 10 Division of Space Technology, Department of Computer Science, Electrical and Space Engineering, Luleå University of Technology , Kiruna, Sweden
- 12 Centro de Astrobiología (INTA-CSIC) , Madrid, Spain
| | | | | | - Alexander V Stepanov
- 1 Space Research Institute IKI , Moscow, Russia
- 3 Department of Physics, Lomonosov Moscow State University , Russia
| | | | | | | | | | - Yurii K Kalinnikov
- 14 National Research Institute for Physicotechnical and Radio Engineering Measurements VNIIFTRI , Mendeleevo, Russia
| | - Yurii S Ivanov
- 15 Main Astronomical Observatory MAO NASU , Kyiv, Ukraine
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8
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Liu W, Li S, Chen S. Computer simulation of random loose packings of micro-particles in presence of adhesion and friction. POWDER TECHNOL 2016. [DOI: 10.1016/j.powtec.2016.08.068] [Citation(s) in RCA: 25] [Impact Index Per Article: 3.1] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/21/2022]
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9
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Chen S, Li S, Liu W, Makse HA. Effect of long-range repulsive Coulomb interactions on packing structure of adhesive particles. SOFT MATTER 2016; 12:1836-1846. [PMID: 26677107 DOI: 10.1039/c5sm02403j] [Citation(s) in RCA: 18] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/05/2023]
Abstract
The packing of charged micron-sized particles is investigated using discrete element simulations based on adhesive contact dynamic model. The formation process and the final obtained structures of ballistic packings are studied to show the effect of interparticle Coulomb force. It is found that increasing the charge on particles causes a remarkable decrease of the packing volume fraction ϕ and the average coordination number 〈Z〉, indicating a looser and chainlike structure. Force-scaling analysis shows that the long-range Coulomb interaction changes packing structures through its influence on particle inertia before they are bonded into the force networks. Once contact networks are formed, the expansion effect caused by repulsive Coulomb forces are dominated by short-range adhesion. Based on abundant results from simulations, a dimensionless adhesion parameter Ad*, which combines the effects of the particle inertia, the short-range adhesion and the long-range Coulomb interaction, is proposed and successfully scales the packing results for micron-sized particles within the latest derived adhesive loose packing (ALP) regime. The structural properties of our packings follow well the recent theoretical prediction which is described by an ensemble approach based on a coarse-grained volume function, indicating some kind of universality in the low packing density regime of the phase diagram regardless of adhesion or particle charge. Based on the comprehensive consideration of the complicated inter-particle interactions, our findings provide insight into the roles of short-range adhesion and repulsive Coulomb force during packing formation and should be useful for further design of packings.
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Affiliation(s)
- Sheng Chen
- Key Laboratory for Thermal Science and Power Engineering of Ministry of Education, Department of Thermal Engineering, Tsinghua University, Beijing 100084, China.
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10
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Liu W, Li S, Baule A, Makse HA. Adhesive loose packings of small dry particles. SOFT MATTER 2015; 11:6492-6498. [PMID: 26186271 DOI: 10.1039/c5sm01169h] [Citation(s) in RCA: 27] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/04/2023]
Abstract
We explore adhesive loose packings of small dry spherical particles of micrometer size using 3D discrete-element simulations with adhesive contact mechanics and statistical ensemble theory. A dimensionless adhesion parameter (Ad) successfully combines the effects of particle velocities, sizes and the work of adhesion, identifying a universal regime of adhesive packings for Ad > 1. The structural properties of the packings in this regime are well described by an ensemble approach based on a coarse-grained volume function that includes the correlation between bulk and contact spheres. Our theoretical and numerical results predict: (i) an equation of state for adhesive loose packings that appear as a continuation from the frictionless random close packing (RCP) point in the jamming phase diagram and (ii) the existence of an asymptotic adhesive loose packing point at a coordination number Z = 2 and a packing fraction ϕ = 1/2(3). Our results highlight that adhesion leads to a universal packing regime at packing fractions much smaller than the random loose packing (RLP), which can be described within a statistical mechanical framework. We present a general phase diagram of jammed matter comprising frictionless, frictional, adhesive as well as non-spherical particles, providing a classification of packings in terms of their continuation from the spherical frictionless RCP.
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Affiliation(s)
- Wenwei Liu
- Key Laboratory for Thermal Science and Power Engineering of Ministry of Education, Department of Thermal Engineering, Tsinghua University, Beijing 100084, China.
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11
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Kinch KM, Bell JF, Goetz W, Johnson JR, Joseph J, Madsen MB, Sohl-Dickstein J. Dust deposition on the decks of the Mars Exploration Rovers: 10 years of dust dynamics on the Panoramic Camera calibration targets. EARTH AND SPACE SCIENCE (HOBOKEN, N.J.) 2015; 2:144-172. [PMID: 27981072 PMCID: PMC5125412 DOI: 10.1002/2014ea000073] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/23/2014] [Revised: 03/09/2015] [Accepted: 03/26/2015] [Indexed: 05/13/2023]
Abstract
The Panoramic Cameras on NASA's Mars Exploration Rovers have each returned more than 17,000 images of their calibration targets. In order to make optimal use of this data set for reflectance calibration, a correction must be made for the presence of air fall dust. Here we present an improved dust correction procedure based on a two-layer scattering model, and we present a dust reflectance spectrum derived from long-term trends in the data set. The dust on the calibration targets appears brighter than dusty areas of the Martian surface. We derive detailed histories of dust deposition and removal revealing two distinct environments: At the Spirit landing site, half the year is dominated by dust deposition, the other half by dust removal, usually in brief, sharp events. At the Opportunity landing site the Martian year has a semiannual dust cycle with dust removal happening gradually throughout two removal seasons each year. The highest observed optical depth of settled dust on the calibration target is 1.5 on Spirit and 1.1 on Opportunity (at 601 nm). We derive a general prediction for dust deposition rates of 0.004 ± 0.001 in units of surface optical depth deposited per sol (Martian solar day) per unit atmospheric optical depth. We expect this procedure to lead to improved reflectance-calibration of the Panoramic Camera data set. In addition, it is easily adapted to similar data sets from other missions in order to deliver improved reflectance calibration as well as data on dust reflectance properties and deposition and removal history.
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Affiliation(s)
- Kjartan M Kinch
- Niels Bohr Institute University of Copenhagen Copenhagen Denmark
| | - James F Bell
- School of Earth and Space Exploration Arizona State University Phoenix Arizona USA
| | - Walter Goetz
- Max Planck Institute for Solar System Research Göttingen Germany
| | - Jeffrey R Johnson
- Applied Physics Laboratory Johns Hopkins University Laurel Maryland USA
| | - Jonathan Joseph
- Department of Astronomy Cornell University Ithaca New York USA
| | - Morten Bo Madsen
- Niels Bohr Institute University of Copenhagen Copenhagen Denmark
| | - Jascha Sohl-Dickstein
- Neural Dynamics and Computation Laboratory Stanford University Stanford California USA
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12
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Lorenz RD, Reiss D. Solar Panel Clearing Events, Dust Devil Tracks, and in-situ Vortex Detections on Mars. ICARUS 2015; 248:162-164. [PMID: 30705464 PMCID: PMC6350794 DOI: 10.1016/j.icarus.2014.10.034] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/09/2023]
Abstract
Spirit rover solar array data, which if publicly-archived would provide a useful window on Mars meteorology, shows dust-clearing events coinciding with the onset of dust devil season in three Mars years. The recurrence interval of 100-700 days is consistent with the extrapolation of Pathfinder and Phoenix vortex encounters indicated by pressure drops of ~6-40 Pa (similar to laboratory measurements of dust lifting threshold) and with observed areas and rates of generation of dust devil tracks on Mars.
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Affiliation(s)
- Ralph D Lorenz
- Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA
| | - Dennis Reiss
- Institut für Planetologie, Westfälische Wilhelms-Universität, Wilhelm-Klemm-Str. 10, 48149 Münster, Germany
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13
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Ruff SW, Farmer JD, Calvin WM, Herkenhoff KE, Johnson JR, Morris RV, Rice MS, Arvidson RE, Bell JF, Christensen PR, Squyres SW. Characteristics, distribution, origin, and significance of opaline silica observed by the Spirit rover in Gusev crater, Mars. ACTA ACUST UNITED AC 2011. [DOI: 10.1029/2010je003767] [Citation(s) in RCA: 125] [Impact Index Per Article: 9.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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14
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Sullivan R, Arvidson R, Bell JF, Gellert R, Golombek M, Greeley R, Herkenhoff K, Johnson J, Thompson S, Whelley P, Wray J. Wind-driven particle mobility on Mars: Insights from Mars Exploration Rover observations at “El Dorado” and surroundings at Gusev Crater. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2008je003101] [Citation(s) in RCA: 220] [Impact Index Per Article: 13.8] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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15
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Bell JF, Rice MS, Johnson JR, Hare TM. Surface albedo observations at Gusev Crater and Meridiani Planum, Mars. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2007je002976] [Citation(s) in RCA: 28] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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16
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Goetz W, Leer K, Gunnlaugsson HP, Bartlett P, Basso B, Bell J, Bertelsen P, Binau CS, Chu PC, Gorevan S, Hansen MF, Hviid SF, Kinch KM, Klingelhöfer G, Kusack A, Madsen MB, Ming DW, Morris RV, Mumm E, Myrick T, Olsen M, Squyres SW, Wilson J, Yen A. Search for magnetic minerals in Martian rocks: Overview of the Rock Abrasion Tool (RAT) magnet investigation on Spirit and Opportunity. ACTA ACUST UNITED AC 2008. [DOI: 10.1029/2006je002819] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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