Search results for "atmosphere [muon]"

showing 10 items of 25 documents

Adaptation to climate change of the French wine industry: a systemic approach – Main outcomes of the project LACCAVE

2018

Présenté au 12. Congreso Internacional Terroir; Taking into account the major economical role and specificities of the French wine industry, adaptation to climate change is a very challenging issue. In 2011, 23 research teams launched a systemic and multidisciplinary program to analyze the impacts from the vine to the region, to define adaptation strategies combining technical, spatial and organizational options and to evaluate the perception by the actors and consumers of climate change issues. Thermal variability was studied at local scale to develop high resolution atmospheric models which better simulate future climate trends. Impacts on growth/developmental conditions and vine response…

0106 biological sciencesmodèle atmosphérique010504 meteorology & atmospheric sciencesmedia_common.quotation_subjectTempérature élevee[SDE.MCG]Environmental Sciences/Global ChangesClimate changethermal behaviorfilière vitivinicole01 natural sciencesMultidisciplinary approachtempérature eleveePerceptionatmosphere modelstratégie d'adaptation[SDV.BV]Life Sciences [q-bio]/Vegetal BiologySystemic approachAdaptation (computer science)Milieux et Changements globauxEnvironmental planninglcsh:Environmental sciences0105 earth and related environmental sciencesmedia_commonStrategic planninglcsh:GE1-350étude prospectiveFutures studiesindice climatique13. Climate actionBusinessadaptation au changement climatiquecomportement thermiqueclimatic index010606 plant biology & botanyWine industry
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First muography of Stromboli volcano

2019

AbstractMuography consists in observing the differential absorption of muons – elementary particles produced through cosmic-ray interactions in the Earth atmosphere – going through the volcano and can attain a spatial resolution of tens of meters. We present here the first experiment of nuclear emulsion muography at the Stromboli volcano. Muons have been recorded during a period of five months by a detector of 0.96 m2 area. The emulsion films were prepared at the Gran Sasso underground laboratory and were analyzed at Napoli, Salerno and Tokyo scanning laboratories. Our results highlight a significant low-density zone at the summit of the volcano with density contrast of 30–40% with respect …

0301 basic medicineDifferential absorptionmuographylcsh:MedicineVolcanologyArticle03 medical and health sciences0302 clinical medicineMuographyStromboliDensity contrastlcsh:SciencegeographyMultidisciplinarygeography.geographical_feature_categoryBedrockmuography; nuclear emulsion; Stromboli; volcanolcsh:RLandslide030104 developmental biologyAtmosphere of EarthGeophysicsvolcanoVolcanonuclear emulsionUnderground laboratorylcsh:QExperimental particle physics030217 neurology & neurosurgeryGeologySeismology
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Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

2012

Atmospheric conditions at the site of a cosmic ray observatory must be known for reconstructing observed extensive air showers. The Global Data Assimilation System (GDAS) is a global atmospheric model predicated on meteorological measurements and numerical weather predictions. GDAS provides altitude-dependent profiles of the main state variables of the atmosphere like temperature, pressure, and humidity. The original data and their application to the air shower reconstruction of the Pierre Auger Observatory are described. By comparisons with radiosonde and weather station measurements obtained on-site in Malargüe and averaged monthly models, the utility of the GDAS data is shown.

AstronomyAtmospheric modelAtmospheric monitoringAtmospheric sciencesCosmic Rays Shower01 natural scienceslaw.inventionData assimilationlawcosmic rays; extensive air showers; atmospheric monitoring; atmospheric modelsDEPENDENCEATMOSFERA (OBSERVAÇÃO)TEMPERATUREPhysics::Atmospheric and Oceanic PhysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]Cascada atmosférica extensaOPTICAL DEPTH[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryAtmospheric temperatureRadiación cósmicaAtmosphere of EarthComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRadiosondeFísica nuclearREFRACTIVE-INDEXAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]MeteorologyAtmospheric MonitoringAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic Rays ShowersEXTENSIVE AIR-SHOWERSCosmic RayAtmósferaWeather stationAtmospheric models0103 physical sciencesExtensive air showers010306 general physicsCosmic raysDETECTORCiencias ExactasPierre Auger ObservatoryAtmospheric models010308 nuclear & particles physicsFísicaAstronomy and Astrophysics13. Climate actionExperimental High Energy PhysicsEMISSION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Column-integrated aerosol optical properties from ground-based spectroradiometer measurements at Barrax (Spain) during the Digital Airborne Spectrome…

2003

[1] The Digital Airborne Imaging Spectrometer Experiment (DAISEX) was carried out for the European Space Agency (ESA) in order to develop the potential of spaceborne imaging spectroscopy for a range of different scientific applications. DAISEX involved simultaneous data acquisitions using different airborne imaging spectrometers over test sites in southeast Spain (Barrax) and the Upper Rhine valley (Colmar, France, and Hartheim, Germany). This paper presents the results corresponding to the columnintegrated aerosol optical properties from ground-based spectroradiometer measurements over the Barrax area during the DAISEX campaign days in the years 1998, 1999, and 2000. The instruments used f…

Atmospheric ScienceRadiació solarImaging spectrometerIrradianceSoil ScienceAquatic ScienceOceanographyGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyRemote sensingAerosolsEcologySpectrometerPaleontologyForestryGeofísicaAerosolImaging spectroscopyGeophysicsAtmosphere of EarthSpectroradiometerSpace and Planetary ScienceVisible rangeEnvironmental science
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2016

Abstract. Aerosols have important impacts on air quality and climate, but the processes affecting their removal from the atmosphere are not fully understood and are poorly constrained by observations. This makes modelled aerosol lifetimes uncertain. In this study, we make use of an observational constraint on aerosol lifetimes provided by radionuclide measurements and investigate the causes of differences within a set of global models. During the Fukushima Dai-Ichi nuclear power plant accident of March 2011, the radioactive isotopes cesium-137 (137Cs) and xenon-133 (133Xe) were released in large quantities. Cesium attached to particles in the ambient air, approximately according to their av…

Atmospheric ScienceRadionuclide010504 meteorology & atmospheric sciences010501 environmental sciencesAtmospheric sciences01 natural sciences7. Clean energyPlumeAerosolchemistry.chemical_compoundAtmosphere of Earthchemistry13. Climate actionTRACERSulfate aerosolSulfateAir quality index0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Comparison of Radiosonde and Remote Sensing Data to Evaluate Convective Forest Fire Risk: The Haines Index

2018

Haines Index (HI) has been associated with convective forest fires risk. Temperatures and humidities in low atmospheric levels are required to compute HI and usually, atmospheric sounding data are used for this purpose. However, spatial and temporal resolutions of these data are coarse and remote sensing data could improve them. Therefore, the aim of this work is to test remote sensing data from the Atmospheric Infrared Sounder (AIRS) instrument on board the EOS Aqua satellite, specifically the Level 2 V6 products (AIRX2RET and AIRS2RET), for this purpose. First, we validated the remote sensing data with radiosonde daytime and nighttime data located in the Iberian Peninsula in 2014. Signifi…

Atmospheric sounding021110 strategic defence & security studiesDaytime010504 meteorology & atmospheric sciences0211 other engineering and technologies02 engineering and technology01 natural scienceslaw.inventionHaines IndexSea surface temperatureAtmosphere of EarthlawAtmospheric Infrared SounderRadiosondeEnvironmental scienceSatellite0105 earth and related environmental sciencesRemote sensingIGARSS 2018 - 2018 IEEE International Geoscience and Remote Sensing Symposium
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Martian zeolites as a source of atmospheric methane

2016

The origin of the martian methane is still poorly understood. A plausible explanation is that methane could have been produced either by hydrothermal alteration of basaltic crust or by serpentinization of ultramafic rocks producing hydrogen and reducing crustal carbon into methane. Once formed, methane storage on Mars is commonly associated with the presence of hidden clathrate reservoirs. Here, we alternatively suggest that chabazite and clinoptilolite, which belong to the family of zeolites, may form a plausible storage reservoir of methane in the martian subsurface. Because of the existence of many volcanic terrains, zeolites are expected to be widespread on Mars and their Global Equival…

Chabazite010504 meteorology & atmospheric sciencesClathrate hydrateFOS: Physical sciences01 natural sciencesMethaneAstrobiologychemistry.chemical_compound0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)BasaltMartianAtmospheric methaneAstronomy and AstrophysicsMars Exploration ProgramAtmosphere of Marschemistry13. Climate actionSpace and Planetary Science[SDU]Sciences of the Universe [physics]Environmental science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph][ SDU ] Sciences of the Universe [physics]Astrophysics - Earth and Planetary Astrophysics
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Evidence of small-scale magnetic concentrations dragged by vortex motion of solar photospheric plasma

2010

Vortex-type motions have been measured by tracking bright points in high-resolution observations of the solar photosphere. These small-scale motions are thought to be determinant in the evolution of magnetic footpoints and their interaction with plasma and therefore likely to play a role in heating the upper solar atmosphere by twisting magnetic flux tubes. We report the observation of magnetic concentrations being dragged towards the center of a convective vortex motion in the solar photosphere from high-resolution ground-based and space-borne data. We describe this event by analyzing a series of images at different solar atmospheric layers. By computing horizontal proper motions, we detec…

ConvectionProper motion:ASTRONOMÍA Y ASTROFÍSICA::Sistema solar [UNESCO]photosphere [Sun]FOS: Physical sciencesAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAConvectionMagnetogramAstrophysics::Solar and Stellar AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPhotosphereUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Sistema solarConvection; Sun: granulation; Sun: photosphere; Magnetic fieldsAstronomy and AstrophysicsMagnetic fluxMagnetic fieldVortexAtmosphere of EarthAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsAstrophysics::Earth and Planetary Astrophysicsgranulation [Sun]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Atmospheric components determination from ground-level measurements during the spectra Barax Campaigns (SPARC) field campaigns

2007

The Surface Processes and Ecosystem Changes Through Response Analysis (SPECTRA) Barrax Campaigns were validation campaigns developed in the framework of the SPECTRA mission in order to verify that the geophysical data products provided by satellite imagery are consistent with the measurements made by independent means. Two campaigns took place in Barrax, Spain, during the summers of 2003 and 2004. This paper presents the results of the characterization of the atmospheric composition from solar radiation, radiosoundings, and lidar measurements. Several potentially interesting situations involving atmospheric layers with different types of aerosols and water content are discussed. The presenc…

Earth observationMeteorologyAtmospheric correction550 - Earth sciencesAtmospheric modelLidarAir mass (astronomy)Atmosphere of EarthRadiative transferGeneral Earth and Planetary SciencesEnvironmental scienceElectrical and Electronic EngineeringAtmospheric opticsRemote sensing
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A numerical study of the Schumann resonances in Mars with the FDTD method

2007

[1] Natural electromagnetic waves generated near the surface by electrostatic discharges in dust storms (dust devils) or by geological activity could be trapped in the resonant cavity formed by the surface and lower ionosphere of Mars, as it occurs on Earth giving rise to Schumann resonances. The finite difference time-domain technique (FDTD) is applied to model the atmosphere of Mars in order to determine Schumann resonant frequencies, and natural electromagnetic fields at the extremely low frequency range (ELF). A numerical tool is provided to analyze the electrical conductivity profile of the Martian atmosphere, with the aim of obtaining Schumann resonance frequencies and their dependenc…

Electromagnetic fieldAtmospheric ScienceSoil ScienceAquatic ScienceOceanographyElectromagnetic radiationAtmosphereOpticsGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Extremely low frequencyEarth-Surface ProcessesWater Science and TechnologyPhysicsEcologySchumann resonancesbusiness.industryPaleontologyForestryMars Exploration ProgramAtmosphere of MarsComputational physicsGeophysicsSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsIonospherebusinessJournal of Geophysical Research: Space Physics
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