Search results for "aves"

showing 10 items of 2443 documents

Zr/Hf ratio and REE behaviour: A coupled indication of lithogenic input in marginal basins and deep-sea brines

2019

Abstract The distribution of dissolved Zr, Hf and Rare Earth Elements (yttrium and lanthanides, hereafter referred to as REE) in the Eastern Mediterranean seawater column was measured in the Kryos basin to evaluate the lithogenic contribution from both Nile River and Sahara and Arabian desert dust. We found dissolved Zr/Hf ratios below the signature of crustal rocks and chondrites; a phenomenon likely driven by the dissolution of the Mn-rich coating of atmospheric dust particles delivered from the desert. In deeper waters, Zr/Hf ratios are clustered close to the signature of crustal rocks and chondrites according to the different Zr and Hf dissolved speciation. The Zr/Hf ratio observed in t…

010504 meteorology & atmospheric sciencesEvaporiteGeochemistrychemistry.chemical_elementYttrium010502 geochemistry & geophysicsOceanography01 natural sciencesDeep seaAnoxic watersWaves and shallow waterOceanographychemistryChondriteSeawaterZr/HfDissolutionGeology0105 earth and related environmental sciencesDeep Sea Research Part II: Topical Studies in Oceanography
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GJ 357 b: A Super-Earth Orbiting an Extremely Inactive Host Star

2020

Aims. In this paper we present a deep X-ray observation of the nearby M dwarf GJ 357 and use it to put constraints on the atmospheric evolution of its planet, GJ 357 b. We also analyse the systematic errors in the stellar parameters of GJ 357 in order to see how they affect the perceived planetary properties. Methods. By comparing the observed X-ray luminosity of its host star, we estimate the age of GJ 357 b as derived from a recent XMM-Newton observation (log Lx [erg s-1] = 25.73), with Lx-age relations for M dwarfs. We find that GJ 357 presents one of the lowest X-ray activity levels ever measured for an M dwarf, and we put a lower limit on its age of 5 Gyr. Using this age limit, we perf…

010504 meteorology & atmospheric sciencesOpacityFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciencesLuminosityPlanet0103 physical sciences010303 astronomy & astrophysicsstars [X rays]Solar and Stellar Astrophysics (astro-ph.SR)physical evolution [Planets and satellites]0105 earth and related environmental sciencesEnvelope (waves)PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Secondary atmosphereSuper-EarthAstronomy and AstrophysicsRadiusPlanet star interactionsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Scienceterrestrial planets [Planets and satellites]atmospheres [Planets and satellites]Astrophysics - Earth and Planetary Astrophysics
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Ray optics for absorbing particles with application to ice crystals at near-infrared wavelengths

2018

Abstract Light scattering by particles large compared to the wavelength of incident light is traditionally solved using ray optics which considers absorption inside the particle approximately, along the ray paths. To study the effects rising from this simplification, we have updated the ray-optics code SIRIS to take into account the propagation of light as inhomogeneous plane waves inside an absorbing particle. We investigate the impact of this correction on traditional ray-optics computations in the example case of light scattering by ice crystals through the extended near-infrared (NIR) wavelength regime. In this spectral range, ice changes from nearly transparent to opaque, and therefore…

010504 meteorology & atmospheric sciencesOpacityspektroskopiaIce crystalsPhysics::OpticsRay optics01 natural sciencesPOLARIZED-LIGHT SCATTERING114 Physical sciencesLight scattering010309 opticsScatteringMEDIAOptics0103 physical sciencesABSORPTIONInhomogeneous wavesCIRRUSray opticsSpectroscopy0105 earth and related environmental sciencesPhysicsta113absorbing mediaRadiationta115Geometrical opticsIce crystalsta114Scatteringbusiness.industryscatteringCLOUDSkiteetRayAtomic and Molecular Physics and OpticsoptiikkaSOLAR-RADIATIONWavelengthMAXWELLS EQUATIONSAbsorbing mediainhomogeneous wavesLight scattering by particlesPHASE MATRIXGEOMETRIC-OPTICSbusinessice crystalsAPPROXIMATION
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Oscillations on Width and Intensity of Slender Ca ii H Fibrils from Sunrise/SuFI

2017

R. Gafeira et. al.

010504 meteorology & atmospheric sciencesPhase (waves)FOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencesMolecular physics0103 physical sciencesWave modeSunriseSun: oscillationsTechniques: imaging spectroscopySun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSolar observatoryoscillations [Sun]imaging spectroscopy [Techniques]Sun: chromosphereAstronomy and AstrophysicsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]Space and Planetary ScienceIntensity (heat transfer)The Astrophysical Journal Supplement Series
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Secondary minerals from salt caves in the Atacama Desert (Chile): a hyperarid and hypersaline environment with potential analogies to the Martian sub…

2017

Over the past 15 years several expeditions by French, American and especially Italian cavers have unveiled over 50 caves in the Cordillera de la Sal (Atacama Desert, Northern Chile). Many of these caves contain a variety of speleothems and minerals, some of which have rarely been observed within karst systems. Most of the secondary deposits in these caves are composed of halite, but also other halide, carbonate, sulphate, nitrate, phosphate, and silicate minerals have been found. Among the sixteen cave mineral species recognized, atacamite, darapskite, blödite, leonite, anhydrite, and especially antarcticite are worth mentioning. In one of the samples an unknown Ca-Sr-bearing chloride miner…

010504 meteorology & atmospheric sciencesQH301-705.5Settore GEO/04 - Geografia Fisica E GeomorfologiaEarth scienceSalt (chemistry)martian010502 geochemistry & geophysics01 natural sciencesAstrobiologyatacamaCaveminerogenesisMinerogenesiBiology (General)Hyperaridity0105 earth and related environmental sciencesEarth-Surface Processescave mineralschemistry.chemical_classificationMartianQE1-996.5Settore GEO/06 - Mineralogiageographygeography.geographical_feature_categoryDesert (philosophy)Mars analoguesMars analogueCave mineralGeologysalt cavescave minerals atacama martianchemistrySalt cavecave minerals salt caves hyperaridity minerogenesis Mars analoguesGeologyInternational Journal of Speleology
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PHYSICS-based retrieval of scattering albedo and vegetation optical depth using multi-sensor data integration

2017

Vegetation optical depth and scattering albedo are crucial parameters within the widely used τ-ω model for passive microwave remote sensing of vegetation and soil. A multi-sensor data integration approach using ICESat lidar vegetation heights and SMAP radar as well as radiometer data enables a direct retrieval of the two parameters on a physics-derived basis. The crucial step within the retrieval methodology is the calculus of the vegetation scattering coefficient KS, where one exact and three approximated solutions are provided. It is shown that, when using the assumption of a randomly oriented volume, the backscatter measurements of the radar provide a sufficient first order estimate and …

010504 meteorology & atmospheric sciencesScattering albedo0208 environmental biotechnologyradiometry02 engineering and technologyretrieval methodologycomputer.software_genre01 natural scienceslaw.inventionlawremote sensing by radarRadaractive-passive microwavesPhysics::Atmospheric and Oceanic PhysicsIndexespassive microwave remote sensingRemote sensingremote sensing by laser beamGeographyLidaroptical radarcrucial parametersmedicine.symptomvegetation scattering coefficientData integrationBackscattervegetation mappingta1171τ-ω modelsoilPhysics::GeophysicsICESat lidar vegetation heightsvegetationmedicineVegetation optical depthbackscatter0105 earth and related environmental sciencesRemote sensingsensor fusionRadiometerScatteringnovel multisensor approachSMAPAlbedoMulti-sensor020801 environmental engineeringradiometer dataVegetation (pathology)multisensor data integration approachcomputerICESatalbedo
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Slow-Mode Magnetoacoustic Waves in Coronal Loops

2021

Rapidly decaying long-period oscillations often occur in hot coronal loops of active regions associated with small (or micro-) flares. This kind of wave activity was first discovered with the SOHO/SUMER spectrometer from Doppler velocity measurements of hot emission lines, thus also often called "SUMER" oscillations. They were mainly interpreted as global (or fundamental mode) standing slow magnetoacoustic waves. In addition, increasing evidence has suggested that the decaying harmonic type of pulsations detected in light curves of solar and stellar flares are likely caused by standing slow-mode waves. The study of slow magnetoacoustic waves in coronal loops has become a topic of particular…

010504 meteorology & atmospheric sciencesSolar activityFOS: Physical sciencesSolar corona01 natural sciencesStanding wave0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesCoronal seismologyPhysicsOscillationOscillations and wavesAstronomy and AstrophysicsCoronal loopLight curveThermal conductionCoronal loopsComputational physicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamics
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Eustasy and sea water Sr composition: application to high-resolution Sr-isotope stratigraphy of Miocene shallow-water carbonates

2007

Oceanic 87 Sr/ 86 Sr-isotope ratios are strongly influenced by rates of silicate weathering and therefore linked not only to glaciation but also to sea-level change. The present study combines analysis of sequence stratigraphy and basin architecture with Sr-isotope stratigraphy in Miocene shallow-water sediments in southern Portugal and Crete (Greece). The common method is to use smoothed global sea water Sr-isotope reference curves but here a different approach is chosen. Instead, measured Sr-isotope curves are correlated with unsmoothed reference curves by identification of similar fluctuations in the order of several 100 kyr. Transgressive intervals are characterized by increasing Sr-iso…

010504 meteorology & atmospheric sciencesStratigraphy550 - Earth sciencesGeologyWeathering010502 geochemistry & geophysics01 natural sciencesSilicateWaves and shallow waterPaleontologychemistry.chemical_compoundStratigraphychemistry13. Climate actionDeglaciationSequence stratigraphySedimentary rock14. Life underwaterChronostratigraphyGeology0105 earth and related environmental sciencesSedimentology
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The tsunami phenomenon

2017

Abstract With human activity increasingly concentrating on coasts, tsunamis (from Japanese tsu = harbour, nami = wave) are a major natural hazard to today’s society. Stimulated by disastrous tsunami impacts in recent years, for instance in south-east Asia (2004) or in Japan (2011), tsunami science has significantly flourished, which has brought great advances in hazard assessment and mitigation plans. Based on tsunami research of the last decades, this paper provides a thorough treatise on the tsunami phenomenon from a geoscientific point of view. Starting with the wave features, tsunamis are introduced as long shallow water waves or wave trains crossing entire oceans without major energy l…

010504 meteorology & atmospheric sciencesSubmarineGeologyAquatic ScienceHazard analysis010502 geochemistry & geophysics01 natural sciencesWaves and shallow waterOceanographyWave shoalingNatural hazardSubmarine pipelineSedimentary rockTsunami earthquakeGeologySeismology0105 earth and related environmental sciencesProgress in Oceanography
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Measuring the electron temperatures of coronal mass ejections with future space-based multi-channel coronagraphs: a numerical test

2018

Context. The determination from coronagraphic observations of physical parameters of the plasma embedded in coronal mass ejections (CMEs) is of crucial importance for our understanding of the origin and evolution of these phenomena. Aims. The aim of this work is to perform the first ever numerical simulations of a CME as it will be observed by future two-channel (visible light VL and UV Ly-α) coronagraphs, such as the Metis instrument on-board ESA-Solar Orbiter mission, or any other future coronagraphs with the same spectral band-passes. These simulations are then used to test and optimize the plasma diagnostic techniques to be applied to future observations of CMEs. Methods. The CME diagno…

010504 meteorology & atmospheric sciencesSun: coronal mass ejections (CMEs)Plasma parametersT-NDASContext (language use)Astrophysics01 natural sciencessymbols.namesakeMethods: data analysis0103 physical sciencesRadiative transferCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsQB Astronomydata analysis [Methods]010303 astronomy & astrophysicsQCQB0105 earth and related environmental sciencesPhysicsUV radiation [Sun]numerical [Methods]Methods: numericalAstronomy and AstrophysicsPlasmaSun: UV radiationPolarization (waves)coronal mass ejections (CMEs) [Sun]Computational physicsQC PhysicsPlasmasSpace and Planetary SciencePhysics::Space PhysicssymbolsMagnetohydrodynamicsDoppler effectAstronomy & Astrophysics
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