Search results for "Climate"

showing 10 items of 4934 documents

Horizontal distribution of copper, nickel and enchytraeid worms in polluted soil

1999

We studied the horizontal distribution of Cu, Ni and enchytraeid worms (Cognettia sphagnetorum, Vejdovsky, Oligochaeta, Enchytraeidae) in forest soil near a Cu–Ni smelter in SW Finland. Soil samples were taken from a polluted site (2 km from the smelter) and a reference area (8 km from the smelter). We used a hierarchical sampling design in the polluted area for studying possible scale-dependent variability in parameters measured, distance between the samples (different scales) being 5, 50 and 500 cm. Distribution of metals was moderately heterogeneous in the polluted soil; coefficient of variances (CV), 26% for Cu and 32% for Ni. Instead, distribution of enchytraeids in the area was highly…

Soil testHealth Toxicology and MutagenesisPopulation010501 environmental sciencesToxicology01 natural sciencesPopulation densityeducation0105 earth and related environmental scienceseducation.field_of_studybiologyEcology04 agricultural and veterinary sciencesGeneral MedicineEnchytraeidae15. Life on landbiology.organism_classificationPollutionSoil contaminationHumus13. Climate actionEnvironmental chemistrySoil water040103 agronomy & agriculture0401 agriculture forestry and fisheriesEnvironmental scienceSpatial variabilityEnvironmental Pollution
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Nano- to Global-Scale Uncertainties in Terrestrial Enhanced Weathering.

2022

Enhanced weathering (EW) is one of the most promising negative emissions technologies urgently needed to limit global warming to at least below 2 °C, a goal recently reaffirmed at the UN Global Climate Change conference (i.e., COP26). EW relies on the accelerated dissolution of crushed silicate rocks applied to soils and is considered a sustainable solution requiring limited technology. While EW has a high theoretical potential of sequestering CO2, research is still needed to provide accurate estimates of carbon (C) sequestration when applying different silicate materials across distinct climates and major soil types in combination with a variety of plants. Here we elaborate on fundamental …

SoilCarbon SequestrationClimate change negative emissions technology global warming carbon sequestration enhanced weathering concrete recyclingClimate ChangeSilicatesSettore ICAR/02 - Costruzioni Idrauliche E Marittime E IdrologiaEnvironmental ChemistryGeneral ChemistryCarbon DioxideWeatherEnvironmental sciencetechnology
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The crucial interactions between climate and soil

2022

Since the birth of soil science, climate has been recognized as a soil-forming factor, along with parent rock, time, topography, and organisms (from which humans were later kept distinct), often prevalent on the other factors on the very long term. But the climate is in turns affected by soils and their management. This paper describes the interrelationships between climate – and its current change – and soil, focusing on each single factor of its formation. Parent material governs, primarily through the particle size distribution, the capacity of soil to retain water and organic matter, which are two main soil-related drivers of the climate. Time is the only unmanageable soil-forming facto…

SoilEnvironmental EngineeringSettore AGR/14 - PedologiaClimate ChangeHumansWaterEnvironmental ChemistryAgricultureBiodiversityLand surface albedo Emissions trading Greenhouse gases (GHG) Pedodiversity Soil organic matter (SOM) Soil water retentionPollutionWaste Management and Disposal
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Small solar system bodies as granular systems

2017

Asteroids and other Small Solar System Bodies (SSSBs) are currently of great scientific and even industrial interest. Asteroids exist as the permanent record of the formation of the Solar System and therefore hold many clues to its understanding as a whole, as well as insights into the formation of planetary bodies. Additionally, SSSBs are being investigated in the context of impact risks for the Earth, space situational awareness and their possible industrial exploitation (asteroid mining). In all these aspects, the knowledge of the geophysical characteristics of SSSB surface and internal structure are of great importance. Given their size, constitution, and the evidence that many SSSBs ar…

Solar SystemSituation awareness[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]Computer sciencePhysicsQC1-999Small solar system bodiesContext (language use)Granular systems01 natural sciencesCelestial mechanicsAstrobiologyTheoretical physics13. Climate actionAsteroidFísica Aplicada0103 physical sciencesFormation and evolution of the Solar System[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010306 general physics010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSSoil mechanicsAsteroid miningEPJ Web of Conferences
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A prospective new diagnostic technique for distinguishing eruptive and noneruptive active regions

2019

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). This work used the DiRAC@Durham facility managed by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk). The equipment was funded by BEIS capital funding via STFC capital grants ST/P002293/1, ST/R002371/1, and ST/S002502/1, Durham University and STFC operations grant ST/R000832/1. DiRAC is part of the National e-Infrastructure. S.L.Y. would like to acknowledge STFC for sup…

Solar coronal mass ejections (310)010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsSolar activityT-NDASLibrary scienceFOS: Physical sciencesSpace weather (2037)Solar coronaSolar activity (1475)Solar flares (1496)01 natural sciencesSolar coronal mass ejectionsSolar corona (1483)0103 physical sciencesmedia_common.cataloged_instanceAstrophysics::Solar and Stellar AstrophysicsQB AstronomyEuropean union010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesmedia_commonQBPhysicsEuropean researchSolar active region magnetic fieldsAstronomy and AstrophysicsSolar active region magnetic fields (1975)Solar magnetic fields (1503)Solar active regionsSolar active regions (1974)QC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSolar flaresSpace and Planetary SciencePhysics::Space Physics
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The Early Spörer Minimum – A Period of Extraordinary Climate and Socio-economic Changes in Western and Central Europe

2016

Abstract. Throughout the last millennium, mankind was affected by prolonged deviations from the climate mean state. While periods like the Maunder Minimum in the 17th century have been assessed in greater detail, earlier cold periods such as the 15th century received much less attention due to the sparse information available. Based on new evidence from different sources ranging from proxy archives to model simulations, it is now possible to provide an end-to-end assessment about the climate state during an exceptionally cold period in the 15th century, the role of internal, unforced climate variability and external forcing in shaping these extreme climatic conditions, and the impacts on an…

Solar minimum010506 paleontology010504 meteorology & atmospheric sciences300 Social sciences sociology & anthropology530 PhysicsFood pricesSubsistence agricultureSeasonalitymedicine.disease01 natural sciencesProxy (climate)13. Climate actionClimatologymedicineFamine570 Life sciences; biologyClimate modelClimate state910 Geography & travel550 Earth sciences & geology900 History0105 earth and related environmental sciences
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Search for Gamma-Ray Emission from the Sun during Solar Minimum with the ARGO-YBJ Experiment

2019

The hadronic interaction of cosmic rays with solar atmosphere can produce high energy gamma-rays. The gamma-ray luminosity is correlated both with the flux of primary cosmic rays and the intensity of the solar magnetic field. The gamma-rays below 200 GeV have been observed by Fermi without any evident energy cutoff. The bright gamma-ray flux above 100 GeV has been detected only during solar minimum. The only available data in the TeV range come from the HAWC observations, however, outside the solar minimum. The ARGO-YBJ data set has been used to search for sub-TeV/TeV gamma-rays from the Sun during the solar minimum from 2008 to 2010, the same time period covered by the Fermi data. A suitab…

Solar minimumSun: generalAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayastroparticle physics; cosmic rays; gamma rays: general; Sun: general7. Clean energy01 natural sciencesAtmospherecosmic rays0103 physical sciencesgeneral [Sun]010303 astronomy & astrophysicsArgocosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysics010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleGamma rayAstronomyastroparticle physicAstronomy and Astrophysicsgamma rays: general13. Climate actionSpace and Planetary Scienceastroparticle physicsHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenageneral [gamma rays]
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Resonant origin for density fluctuations deep within the Sun: helioseismology and magneto-gravity waves

2003

We analyze helioseismic waves near the solar equator in the presence of magnetic fields deep within the solar radiative zone. We find that reasonable magnetic fields can significantly alter the shapes of the wave profiles for helioseismic g-modes. They can do so because the existence of density gradients allows g-modes to resonantly excite Alfven waves, causing mode energy to be funnelled along magnetic field lines, away from the solar equatorial plane. The resulting wave forms show comparatively sharp spikes in the density profile at radii where these resonances take place. We estimate how big these waves might be in the Sun, and perform a first search for observable consequences. We find …

Solar neutrinoFOS: Physical sciencesAstrophysicsAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHelioseismology010303 astronomy & astrophysicsSolar equatorPhysics010308 nuclear & particles physicsGravitational waveAstrophysics (astro-ph)FísicaAstronomy and AstrophysicsObservableRadiation zoneMagnetic fieldHigh Energy Physics - PhenomenologyAmplitude13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary Astrophysics
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Spatial Analysis, Cartography and Climate

2010

International audience

Spatial Analysis[SHS.GEO] Humanities and Social Sciences/GeographyClimate[SHS.GEO]Humanities and Social Sciences/GeographyComputingMilieux_MISCELLANEOUSInterpolation[ SHS.GEO ] Humanities and Social Sciences/Geography
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New insights into the neolithisation process in southwest Europe according to spatial density analysis from calibrated radiocarbon dates

2017

The agricultural way of life spreads throughout Europe via two main routes: the Danube corridor and the Mediterranean basin. Current archaeological literature describes the arrival to the Western Mediterranean as a rapid process which involves both demic and cultural models, and in this regard, the dispersal movement has been investigated using mathematical models, where the key factors are time and space. In this work, we have created a compilation of all available radiocarbon dates for the whole of Iberia, in order to draw a chronological series of maps to illustrate temporal and spatial patterns in the neolithisation process. The maps were prepared by calculating the calibrated 14C date …

Spatial densityMediterranean climate010506 paleontologyArcheology060102 archaeology06 humanities and the arts01 natural sciencesMediterranean BasinPrehistòrialaw.inventionPaleontologyKey factorslawAnthropologySpatial ecologyBiological dispersal0601 history and archaeologyRadiocarbon datingPhysical geographyGeologyMesolithic0105 earth and related environmental sciences
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