Search results for "LoRa"

showing 10 items of 2828 documents

New records of Asteraceae for the non-native flora of Tunisia and north Africa with some nomenclatural remarks

2022

International audience; Sixteen new Asteraceae are added to the non-indigenous flora of Tunisia. Six of them (Dimorphotheca ecklonis, Gaillardia pulchella, Gazania linearis var. linearis, Guizotia abyssinica, Rudbeckia triloba and Tithonia diversifolia) are also new for the flora of North Africa. Chrysanthemum morifolium is here first reported for the Mediterranean Basin. Seven genera (Argyranthemum, Bidens, Dimorphotheca, Gaillardia, Guizotia, Rudbeckia and Tithonia) are recorded for the first time for the vascular flora of Tunisia. Most of these species escaped from gardens and pots and became casual along roadsides and/or disturbed areas after cypsela dispersion (except for Chrysanthemum…

AsteroideaeCompositaeEcologySettore BIO/02 - Botanica SistematicaPlant Science[SDV.BV.BOT]Life Sciences [q-bio]/Vegetal Biology/Botanicsalien flora[SDV.BID.SPT]Life Sciences [q-bio]/Biodiversity/Systematics Phylogenetics and taxonomynaturalizationAlien flora[SDV.EE.ECO]Life Sciences [q-bio]/Ecology environment/EcosystemsSettore BIO/03 - Botanica Ambientale E Applicatatypification.Typification.Typification[SDE.BE]Environmental Sciences/Biodiversity and EcologyEcology Evolution Behavior and SystematicsCichorioideaeNaturalization
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Report of the COSPAR Mars special regions colloquium

2010

International audience; In this paper we present the findings of a COSPAR Mars Special Regions Colloquium held in Rome in 2007. We review and discuss the definition of Mars Special Regions, the physical parameters used to define Mars Special Regions, and physical features on Mars that can be interpreted as Mars Special Regions. We conclude that any region experiencing temperatures > -25 degrees C for a few hours a year and a water activity > 0.5 can potentially allow the replication of terrestrial microorganisms. Physical features on Mars that can be interpreted as meeting these conditions constitute a Mars Special Region. Based on current knowledge of the martian environment and the conser…

Atmospheric Science010504 meteorology & atmospheric sciencesPlanetary protectionLiquid waterAerospace EngineeringTerrainBACTERIAL-ACTIVITY01 natural sciencesSPACECRAFT SURFACESAstrobiologyWater-vaporSouth-pole snow0103 physical sciencesBacterial activitySpace research010303 astronomy & astrophysicsBacterial activity0105 earth and related environmental sciencesMartianCommittee on Space ResearchCOSPAR mars special regions colloquiumNear-surfaceAstronomy and AstrophysicsMars Exploration Program15. Life on landGround ice[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]GeophysicsLiquid water13. Climate actionSpace and Planetary ScienceGeneral Earth and Planetary SciencesHigh obliquitySea-iceUpper martian surfaceSpace-craft surfacesGeology
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A spatially consistent downscaling approach for SMOS using an adaptive window

2017

The European Space Agency (ESA)'s Soil Moisture and Ocean Salinity (SMOS) is the first spaceborne mission using L-band radiometry to monitor the Earth's global surface soil moisture (SM). After more than 7 years in orbit, many studies have contributed to improve the quality and applicability of SMOS-derived SM maps. In this research, a novel downscaling algorithm for SMOS is proposed to obtain high-resolution (HR) SM maps at 1 km (L4), from the ∼40 km native resolution of the instrument. This algorithm introduces the concept of a shape adaptive moving window as an improvement of the current semi-empirical downscaling approach at SMOS Barcelona Expert Center, based on the “universal triangle…

Atmospheric ScienceBrightnessTeledeteccióMean squared error010504 meteorology & atmospheric sciencesREMEDHUS0211 other engineering and technologiesHigh resolution02 engineering and technology01 natural sciencesNormalized Difference Vegetation IndexBECComputers in Earth SciencesImage resolution021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensingNative resolutionAdaptive moving windowLow resolutionMoving windowRemote sensing:Enginyeria de la telecomunicació::Radiocomunicació i exploració electromagnètica::Teledetecció [Àrees temàtiques de la UPC]Orbit (dynamics)RadiometryEnvironmental scienceSpatial variabilitySoil moistureSòls -- HumitatDownscalingSMOS
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FIDO science payload simulating the Athena Payload

2002

[1] The Jet Propulsion Laboratory's Field Integrated Development and Operations rover (FIDO) emulates and tests operational rover capabilities for advanced Mars rover missions, such as those originally planned for the Mars Surveyor 2001 Rover and currently planned for the Athena Payload on the Mars Exploration Rovers scheduled for launch in 2003. This paper describes FIDO's science instrument payload, which is fully integrated with rover hardware and software. Remote science teams visualize instrument suite data and generate FIDO commands using the Web Interface for Telescience. FIDO's instrument suite has been used in terrestrial laboratory and field tests to simulate Mars operations, to t…

Atmospheric ScienceComputer scienceSoil ScienceAquatic ScienceOceanographyExploration of Marslaw.inventionSoftwareGeochemistry and PetrologylawEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyRemote sensingEcologySpectrometerbusiness.industryPaleontologyForestryMars Exploration ProgramRobot end effectorMars roverGeophysicsStereo imagingSpace and Planetary ScienceRadiancebusinessJournal of Geophysical Research: Planets
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Opportunity Mars Rover mission: Overview and selected results from Purgatory ripple to traverses to Endeavour crater

2011

Opportunity has been traversing the Meridiani plains since 25 January 2004 (sol 1), acquiring numerous observations of the atmosphere, soils, and rocks. This paper provides an overview of key discoveries between sols 511 and 2300, complementing earlier papers covering results from the initial phases of the mission. Key new results include (1) atmospheric argon measurements that demonstrate the importance of atmospheric transport to and from the winter carbon dioxide polar ice caps; (2) observations showing that aeolian ripples covering the plains were generated by easterly winds during an epoch with enhanced Hadley cell circulation; (3) the discovery and characterization of cobbles and boul…

Atmospheric ScienceEcologyEarth sciencePaleontologySoil ScienceMars exploration roverForestryAquatic ScienceOceanographyAstrobiologyMars roverGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)PurgatoryGeologyEarth-Surface ProcessesWater Science and Technology
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Spirit Mars Rover Mission: Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

2010

Spirit Mars Rover Mission : Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

Atmospheric ScienceEcologyEarth sciencePaleontologySoil ScienceMars exploration roverForestryMars Exploration ProgramAquatic ScienceOceanographyExploration of MarsHavenAstrobiologyMars roverGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Meteorites on Mars observed with the Mars Exploration Rovers

2008

[1] Reduced weathering rates due to the lack of liquid water and significantly greater typical surface ages should result in a higher density of meteorites on the surface of Mars compared to Earth. Several meteorites were identified among the rocks investigated during Opportunity's traverse across the sandy Meridiani plains. Heat Shield Rock is a IAB iron meteorite and has been officially recognized as “Meridiani Planum.” Barberton is olivine-rich and contains metallic Fe in the form of kamacite, suggesting a meteoritic origin. It is chemically most consistent with a mesosiderite silicate clast. Santa Catarina is a brecciated rock with a chemical and mineralogical composition similar to Bar…

Atmospheric ScienceEcologyPaleontologySoil ScienceForestryMars Exploration ProgramAquatic ScienceOceanographyIron meteoriteStrewn fieldAstrobiologyKamaciteMesosideriteGeophysicsImpact craterMeteoriteSpace and Planetary ScienceGeochemistry and PetrologyChondriteEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Evidence for montmorillonite or its compositional equivalent in Columbia Hills, Mars

2007

During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’’ encountered several similar samples that are distinctly different from Martian meteorites and known Gusev crater soils, rocks, and sediments. Occurring in a variety of contexts and locations, these ‘‘Independence class’’ samples are rough-textured, iron-poor (equivalent FeO 4 wt%), have high Al/Si ratios, and often contain unexpectedly high concentrations of one or more minor or trace elements (including Cr, Ni, Cu, Sr, and Y). Apart from accessory minerals, the major component common to these samples has a compositional profile of major and minor elements whic…

Atmospheric ScienceGeochemistryMarsSoil ScienceMineralogymontmorilloniteAquatic ScienceOceanographychemistry.chemical_compoundImpact craterGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)chemical compositionEarth-Surface ProcessesWater Science and TechnologyGusevMineralEcologyPaleontologyForestryColumbia HillsclayMars Exploration ProgramMars explorationSilicateGeophysicsMontmorilloniteMeteoritechemistrySpace and Planetary ScienceroverGusev CraterSoil horizonClay mineralsGeologyJournal of Geophysical Research
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Depth selective Mössbauer spectroscopy: Analysis and simulation of 6.4 keV and 14.4 keV spectra obtained from rocks at Gusev Crater, Mars, and layere…

2008

[1] The miniaturized Mossbauer spectrometer (MIMOS) II Mossbauer spectrometers on the Mars Exploration Rovers (MER) simultaneously obtained 6.4 keV and 14.4 keV Mossbauer spectra from rock and soil targets. Because photons with lower energy have a shallower penetration depth, 6.4 keV spectra contain more mineralogical information about the near-surface region of a sample than do 14.4 keV spectra. The influence of surface layers of varying composition and thickness on Mossbauer spectra was investigated by Monte Carlo simulation and by measurement using a copy of the MER MIMOS II instrument and samples with one or two layers of known thicknesses. Thin sections of minerals or metallic Fe foil …

Atmospheric ScienceMaterials scienceMonte Carlo methodSoil ScienceMineralogyAquatic Scienceengineering.materialOceanographyPhysics::GeophysicsGeochemistry and PetrologyMössbauer spectroscopyEarth and Planetary Sciences (miscellaneous)Surface layerPenetration depthEarth-Surface ProcessesWater Science and TechnologyThin layersOlivineEcologySpectrometerPaleontologyForestryMars Exploration ProgramGeophysicsSpace and Planetary ScienceengineeringJournal of Geophysical Research
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Overview of the magnetic properties experiments on the Mars Explorations Rovers

2009

[1] The Mars Exploration Rovers have accumulated airborne dust on different types of permanent magnets. Images of these magnets document the dynamics of dust capture and removal over time. The strongly magnetic subset of airborne dust appears dark brown to black in Panoramic Camera (Pancam) images, while the weakly magnetic one is bright red. Images returned by the Microscopic Imager reveal the formation of magnetic chains diagnostic of magnetite-rich grains with substantial magnetization (>8 Am2 kg−1). On the basis of Mossbauer spectra the dust contains magnetite, olivine, pyroxene, and nanophase oxides in varying proportions, depending on wind regime and landing site. The dust contains a …

Atmospheric ScienceSoil ScienceMineralogyPyroxeneAquatic Scienceengineering.materialOceanographychemistry.chemical_compoundMagnetizationGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyMagnetiteBasaltOlivineEcologySpinelPaleontologyForestryMars Exploration Programequipment and suppliesSilicateGeophysicschemistrySpace and Planetary ScienceengineeringGeology
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