Search results for "Climate"

showing 10 items of 4934 documents

1400 years of man-environment interactions and soil evolution in the Saint-Mont mountain (Remiremont, Vosges)

2021

International audience; The SolHoM(a) project aims at determining the degree of landscape anthropisation in the Fossard massif (Remiremont, Vosges, France) by estimating the impact of past human occupations on current soils. Nowadays, a forest covers this relatively inhospitable mountain (hard climate, steep slopes, acid soils ...), but some remains suggest human presence for at least 1400 years.The Saint-Mont is a variscan orogenic granitic summit (height 672m) with valuable preserved archaeological relics, located south of the Fossard. At the top was founded the monasterium Habendum (from the 7th century to the French Revolution), which potentially comes after a late-antic castrum.Further…

anthropisation gradientgeographers[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SDU.STU.GM] Sciences of the Universe [physics]/Earth Sciences/Geomorphologypedology[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and PrehistoryLiDAR data analysissteep slopes[SDV.SA.SDS]Life Sciences [q-bio]/Agricultural sciences/Soil studyarchaeologists[SDE.ES]Environmental Sciences/Environmental and Society[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentarcheologyA relatively inhospitable mountain: -hard climate-nowadays covered by forests. Joint work involving soil scientists[SDE.ES] Environmental Sciences/Environmental and Society[SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology[SDV.SA.SDS] Life Sciences [q-bio]/Agricultural sciences/Soil studygeologists and computer scientists[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentVosges mountains-on acid soils developed from a granitic rock
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Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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Ecology and extent of freshwater browning - What we know and what should be studied next in the context of global change

2022

Water browning or brownification refers to increasing water color, often related to increasing dissolved organic matter (DOM) and carbon (DOC) content in freshwaters. Browning has been recognized as a significant physicochemical phenomenon altering boreal lakes, but our understanding of its ecological consequences in different freshwater habitats and regions is limited. Here, we review the consequences of browning on different freshwater habitats, food webs and aquatic-terrestrial habitat coupling. We examine global trends of browning and DOM/DOC, and the use of remote sensing as a tool to investigate browning from local to global scales. Studies have focused on lakes and rivers while seldo…

aquatic-terrestrial couplingliuennut orgaaninen hiili0106 biological sciencesFood ChainEnvironmental Engineering010504 meteorology & atmospheric sciencesvesien tila01 natural scienceswetland networkglobal browningremote sensingkosteikotRiversAnimalsEnvironmental Chemistry14. Life underwaterWaste Management and DisposalEcosystemvedenväri0105 earth and related environmental sciences010604 marine biology & hydrobiology15. Life on landdissolved organic carbonInvertebratesPollutionCarbon6. Clean waterLakes13. Climate actionfood webskaukokartoitusravintoverkotScience of The Total Environment
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Dust environment of an airless object: A phase space study with kinetic models

2016

Abstract The study of dust above the lunar surface is important for both science and technology. Dust particles are electrically charged due to impact of the solar radiation and the solar wind plasma and, therefore, they affect the plasma above the lunar surface. Dust is also a health hazard for crewed missions because micron and sub-micron sized dust particles can be toxic and harmful to the human body. Dust also causes malfunctions in mechanical devices and is therefore a risk for spacecraft and instruments on the lunar surface. Properties of dust particles above the lunar surface are not fully known. However, it can be stated that their large surface area to volume ratio due to their irr…

asteroidsDusty plasma010504 meteorology & atmospheric sciencesPlasma parametersta221ta1171plasma–surface interactionPlasma-surface interactionElectronAstrophysics01 natural sciences7. Clean energyInterplanetary dust cloud0103 physical scienceskinetic particle simulationsta216Moon010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsta115ta213ta114Astronomy and AstrophysicsPlasmaComputational physicsspace plasmaSolar windSurface-area-to-volume ratio13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysical plasmadustAstrophysics::Earth and Planetary AstrophysicsPlanetary and Space Science
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The Gaia-ESO Survey: The origin and evolution of s-process elements

2018

Context. Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations. These trends provide important constraints on stellar and Galactic evolution and they need to be confirmed with large and statistically significant samples of stars spanning wide age and distance intervals. Aims. We aim to trace the abundance patterns and the time evolution of five s-process elements - two belonging to the first peak, Y and Zr, and three belonging to the second peak, Ba, La, and Ce - using the Gaia-ESO IDR5 results for open clusters and disc stars. Methods. From the UVES spectra of cluster member stars, we determined the ave…

astro-ph.GAMetallicityFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: diskAstronomi astrofysik och kosmologiAbundance (ecology)QB4600103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsDisc010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgeneral [Open clusters and associations][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsOpen clusters and associations: generalAstrophysics - Astrophysics of GalaxiesStarsAbundances [Galaxy][SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesAstrophysics::Earth and Planetary AstrophysicsDisk [Galaxy]s-processOpen cluster
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Neutral Iron Emission Lines From The Day-side Of KELT-9b -- The GAPS Programme With HARPS-N At TNG XX

2020

We present the first detection of atomic emission lines from the atmosphere of an exoplanet. We detect neutral iron lines from the day-side of KELT-9b (Teq $\sim$ 4, 000 K). We combined thousands of spectrally resolved lines observed during one night with the HARPS-N spectrograph (R $\sim$ 115, 000), mounted at the Telescopio Nazionale Galileo. We introduce a novel statistical approach to extract the planetary parameters from the binary mask cross-correlation analysis. We also adapt the concept of contribution function to the context of high spectral resolution observations, to identify the location in the planetary atmosphere where the detected emission originates. The average planetary li…

astro-ph.SR010504 meteorology & atmospheric sciencesContinuum (design consultancy)FOS: Physical sciencesContext (language use)Astrophysics01 natural sciencesExoplanet atmospheres; Exoplanet atmospheric composition; High resolution spectroscopyAtmosphereHigh resolution spectroscopy0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumSpectral resolution010303 astronomy & astrophysicsSpectrographInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Settore FIS/05Astronomy and AstrophysicsExoplanetAstrophysics - Solar and Stellar AstrophysicsExoplanet atmospheric composition13. Climate actionSpace and Planetary Scienceastro-ph.EPAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Earth and Planetary AstrophysicsExoplanet atmospheresastro-ph.IM
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Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection

2020

Predicting the large-scale eruptions from the solar corona and their propagation through interplanetary space remains an outstanding challenge in solar- and helio-physics research. In this article, we describe three dimensional magnetohydrodynamic simulations of the inner heliosphere leading up to and including the extreme interplanetary coronal mass ejection (ICME) of 23 July 2012, developed using the code PLUTO. The simulations are driven using the output of coronal models for Carrington rotations 2125 and 2126 and, given the uncertainties in the initial conditions, are able to reproduce an event of comparable magnitude to the 23 July ICME, with similar velocity and density profiles at 1 …

astro-ph.SRSpace weather010504 meteorology & atmospheric sciencesMHDSolar windSTORMFOS: Physical sciencesMagnitude (mathematics)Context (language use)PROPAGATIONAstronomy & AstrophysicsDisturbancesSpace weatherPROTON01 natural sciencesEVENTSMagnetohydrodynamicsPhysics - Space Physicsphysics.plasm-ph0201 Astronomical and Space Sciences0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsScience & TechnologySUNAstronomy and AstrophysicsARRIVALGeophysicsEVOLUTIONSpace Physics (physics.space-ph)Physics - Plasma PhysicsPlasma Physics (physics.plasm-ph)PlutoSolar windAstrophysics - Solar and Stellar Astrophysicsphysics.space-ph13. Climate actionSpace and Planetary ScienceDragPhysical Sciencesastro-ph.EPMagnetohydrodynamicsInterplanetary coronal mass ejectionsHeliosphereAstrophysics - Earth and Planetary AstrophysicsSolar Physics
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Ilmasto ja sen määräämät luonnonolot Suomen asutuksen ja maatalouden historiassa

2012

asutushistoriaadaptation to boreal climateboreal lakes and historyNordic settlementväestöboreal climate and populationväestönmuutoksetmaankäyttöluontoilmastonmuutoksetasutusiron and agriculturemaatalousväestöhistoriaboreaalinen ilmastovyöhykeilmastovyöhykkeetSuomiilmastoboreal climate and agricultureviljanviljelyboreal climate and land use
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Perceived Coach-Created Motivational Climates as Predictors of Athletes' Goal Reengagement: The Mediational Role of Goal Motives.

2021

Athletes have to face several challenges during the sport season, and one of them could involve dealing with unattainable goals. In these situations, being able to reengage in other goals as a form of goal adjustment and in response to contextual demands is adaptive. According to previous literature, some aspects of the athletes’ social context, such as coach-created motivational climates, could encourage more adaptive responses in athletes, and so it is possible that these climates would also promote athletes’ goal regulation and goal reengagement. The purpose of this study was twofold: to analyze whether athletes’ perception of empowering and disempowering climates were related to their g…

athletesPsicologia socialmotivesmotivational climatePsychologygoalsdisempowering climateempowering climateGeneral PsychologyreengagementBF1-990Original ResearchFrontiers in psychology
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L'Oscillation de Madden-Julian et la variabilité pluviométrique régionale en Afrique Subsaharienne

2007

The role of the Madden-Julian Oscillation ("MJO") on rainfall variability in Sub-Saharan Africa is examined, based on daily rain-gauge records and the NCEP-DOE AMIP-II reanalyses. The convective and dynamical signal associated with the MJO is extracted using two differing methodologies, the BMRC daily indices (Wheeler & Hendon 2004) on the one hand, and a Local Mode Analysis ("LMA", Goulet & Duvel 2000) on the other hand. The temporal variability of the MJO (in terms of period, amplitude, seasonality and location of the convective anomalies) is first analysed. Though the overall amplitude of the signal is not related to El Niño, the oscillations occurring under El Niño (La Niña) conditions …

atmospheric <br />dynamicsintraseasonal variabilityinteractions d'échelleSub-Saharan Africavariabilité intrasaisonnièrerainfall<br />dynamique atmosphériqueclimate diagnosticAfrique Subsaharienne[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/Climatology[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatologydiagnostic climatiqueMadden-Julian Oscillationpluviométriescale interactions[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyOscillation de Madden-Julian
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