Search results for "Pact"

showing 10 items of 2355 documents

The accretion flow to the intermittent accreting ms pulsar, HETE J1900.1-2455, as observed by XMM-Newton and RXTE

2012

We present a study of the accretion flow to the intermittent accreting millisecond pulsar, HETE J1900.1-2455, based on observations performed simultaneously by XMM-Newton and RXTE. The 0.33-50 keV spectrum is described by the sum of a hard Comptonized component originated in an optically thin {\tau}~1 corona, a soft kTin~0.2 keV component interpreted as accretion disc emission, and of disc reflection of the hard component. Two emission features are detected at energies of 0.98(1) and 6.58(7) keV, respectively. The latter is identified as K{\alpha} transition of Fe XXIII-XXV. A simultaneous detection in EPIC-pn, EPIC-MOS2, and RGS spectra favours an astrophysical origin also for the former, …

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsCompact star01 natural sciencesSpectral lineidentification line: profiles stars: neutron pulsars: individual: HETE J1900.1-2455 X-rays: binaries [line]GravitationSettore FIS/05 - Astronomia E AstrofisicaMillisecond pulsar0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsline: identification line: profiles stars: neutron pulsars: individual: HETE J1900.1-2455 X-rays: binariesAstronomyAstronomy and AstrophysicsRadiusAccretion (astrophysics)Neutron starAmplitudeSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Comparison of the H-alpha circumstellar disks in Be/X-ray binaries and Be stars

2000

We present a comparative study of the circumstellar disks in Be/X-ray binaries and isolated Be stars based upon the H-alpha emission line. From this comparison it follows that the overall structure of the disks in the Be/X-ray binaries is similar to the disks of other Be stars, i.e. they are axisymmetric and rotationally supported. The factors for the line broadening (rotation and temperature) in the disks of the Be stars and the Be/X-ray binaries seem to be identical. However, we do detect some intriguing differences between the envelopes. On average, the circumstellar disks of the Be/X-ray binaries are twice as dense as the disks of the isolated Be stars. The different distribution of the…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsCompact starRotationUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsEmissionX-raysAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics::Galaxy AstrophysicsLine (formation)PhysicsBinariesAstrophysics (astro-ph)X-rayAstronomy and AstrophysicsCircumstellar matterStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]StarsFull width at half maximumStars ; Emission ; Be star ; Circumstellar matter ; Binaries ; X-raysSpace and Planetary ScienceBe starH-alphaAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Indications of non-conservative mass-transfer in AMXPs

2019

Context. Since the discovery of the first Accreting Millisecond X-ray Pulsar SAX J1808.4-3658 in 1998, the family of these sources kept growing on. Currently, it counts 22 members. All AMXPs are transients with usually very long quiescence periods, implying that mass accretion rate in these systems is quite low and not constant. Moreover, for at least three sources, a non-conservative evolution was also proposed. Aims. Our purpose is to study the long term averaged mass-accretion rates in all the Accreting Millisecond X-ray Pulsars discovered so far, to investigate a non-conservative mass-transfer scenario. Methods. We calculated the expected mass-transfer rate under the hypothesis of a con…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsCompact star01 natural sciencesLuminositystars: neutronX-rays: binariesPulsarpulsars: general0103 physical sciencesX-rays: individuals: IGR J17498−2921X-rays: individuals: IGR J17498-2921010303 astronomy & astrophysicsX-rays: individuals: XTE J1814−338PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsX-rays: binarieX-rays: individuals: XTE J1814-338Radiation pressureSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Magnetic dipole
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Measurement of the distributions of event-by-event flow harmonics in lead-lead collisions at = 2.76 TeV with the ATLAS detector at the LHC

2013

We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, DIP and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW, Poland; GRICES and FCT, Portu…

Atlas detectorUnfolding01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Heavy-ion collisionNaturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)RELATIVISTIC HEAVY-ION COLLISIONSNuclear ExperimentNuclear ExperimentQCunfoldingPhysicsLarge Hadron ColliderAtlas (topology)4. EducationSettore FIS/01 - Fisica SperimentaleEvent-By-Event FluctuationElliptic flowHeavy-Ion CollisionsHarmonic FlowCharged particlehadron-hadron scattering; harmonic flow; event-by-event fluctuation; unfolding; heavy-ion collisionHarmonicsImpact parameterNatural Sciencesharmonic flowParticle Physics - ExperimentNuclear and High Energy PhysicsParticle physicsCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesComputer Science::Digital Libraries530Nuclear physics0103 physical sciencesHeavy ion collisionsddc:530Rapidity010306 general physicsevent-by-event fluctuationCiencias ExactasScience & TechnologyHadron-Hadron Scattering010308 nuclear & particles physicsFísicaheavy ion collisionHeavy-ion collision; harmonic flow; event-by-event fluctuation; unfolding; Hadron-Hadron Scattering
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Controlling Factors of the Climate

1988

Since climate represents the characteristic biospheric conditions at a location or area, it chiefly results from the varying solar and atmospheric moisture and circulation conditions over space and time. Climate at any space or time level is, therefore, represented by certain expressions of the various atmospheric elements, which are concerned with radiation, temperature, sunshine, precipitation and others. The superior impact of the atmosphere upon climate is governed by various factors which control the climate; these climate-controlling factors are, in the widest sense, of a topographical nature (see Sects. 2.1–2.3). Additionally, seasons will be considered as a climate-controlling facto…

Atmospheregeographygeography.geographical_feature_categoryAtmospheric moistureClimate impactClimatologyEnvironmental scienceTime levelPrecipitationScale (map)Pacific oceanMountain range
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Bias correction of dynamically downscaled precipitation to compute soil water deficit for explaining year-to-year variation of tree growth over north…

2017

This paper documents the accuracy of a post-correction method applied to precipitation regionalized by the Weather Research and Forecasting (WRF) Regional Climate Model (RCM) for improving simulated rainfall and feeding impact studies. The WRF simulation covers Burgundy (northeastern France) at a 8-km resolution and over a 20-year long period (1989–2008). Previous results show a strong deficiency of the WRF model for simulating precipitation, especially when convective processes are involved. In order to reduce such biases, a Quantile Mapping (QM) method is applied to WRF-simulated precipitation using the mesoscale atmospheric analyses system SAFRAN («Système d'Analyse Fournissant des Rense…

Atmospheric Science010504 meteorology & atmospheric sciences0208 environmental biotechnologyméthode de correction02 engineering and technologybourgogneCOMMON BEECH01 natural sciencesCiencias de la Tierra y relacionadas con el Medio AmbienteWater balanceREGIONAL CLIMATE MODELLINGGlobal and Planetary Changedéficit hydriqueForestry[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologyClimatologyWATER BALANCECommon beechSOIL WATER DEFICITFrance[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyCIENCIAS NATURALES Y EXACTASforêt tempéréeWRFMesoscale meteorology[ SDV.SA.SDS ] Life Sciences [q-bio]/Agricultural sciences/Soil study[SDV.SA.SDS]Life Sciences [q-bio]/Agricultural sciences/Soil studySpatial distributionDOUGLAS-FIRmedicineREGIONAL CLIMATE-CHANGE; ERA-INTERIM REANALYSIS; POTENTIAL IMPACT; TEMPERATE FOREST; FAGUS-SYLVATICA; SEVERE DROUGHT; MODEL; RESPONSES; SYSTEM; PROJECTIONSPrecipitationmodèle climatique[SDU.STU.HY]Sciences of the Universe [physics]/Earth Sciences/Hydrologyclimatologie régionaleWater balanceSoil water deficit0105 earth and related environmental sciencesQuantile mappingclimatprécipitationDouglas-firQUANTILE MAPPINGnord est de la France15. Life on landSeasonalitymedicine.disease020801 environmental engineering13. Climate actionWeather Research and Forecasting ModelSoil waterEnvironmental scienceClimate modelMeteorología y Ciencias Atmosféricas[ SDU.STU.HY ] Sciences of the Universe [physics]/Earth Sciences/HydrologyAgronomy and Crop ScienceRegional climate modelling
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Intense magmatic degassing through the lake of Copahue volcano, 2013–2014

2015

Here we report on the first assessment of volatile fluxes from the hyperacid crater lake hosted within the summit crater of Copahue, a very active volcano on the Argentina-Chile border. Our observations were performed using a variety of in situ and remote sensing techniques during field campaigns in March 2013, when the crater hosted an active fumarole field, and in March 2014, when an acidic volcanic lake covered the fumarole field. In the latter campaign, we found that 566 to 1373 t d -1 of SO 2 were being emitted from the lake in a plume that appeared largely invisible. This, combined with our derived bulk plume composition, was converted into flux of other volcanic species (H 2 O ~ 1098…

Atmospheric Science010504 meteorology & atmospheric sciencesEarth scienceGeochemistrySoil ScienceAquatic ScienceOceanography010502 geochemistry & geophysics01 natural sciencesCiencias de la Tierra y relacionadas con el Medio AmbienteAtmosphereVulcanologíaFlux (metallurgy)Impact craterGeochemistry and PetrologyCrater lakeEarth and Planetary Sciences (miscellaneous)COPAHUECopahue volcanic lake degassingGeophysicCiencias Exactas y NaturalesChemical compositionWater Science and Technology0105 earth and related environmental sciencesvolcanic lakegeographyMagmatic gasesgeography.geographical_feature_categoryEcologyCopahuePaleontologydegassingForestryFumarolePlumeDEGASSINGGeophysicsVolcano13. Climate actionSpace and Planetary ScienceEarth-Surface ProcesseCopahue volcanovolatile flux from crater lakeCIENCIAS NATURALES Y EXACTASGeologyVOLCANIC LAKEJournal of Geophysical Research: Solid Earth
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Mg/Ca ratios in coralline algae record northwest Atlantic temperature variations and North Atlantic Oscillation relationships

2010

Climate variability in the North Atlantic has been linked in part to the North Atlantic Oscillation (NAO). The NAO influences marine ecosystems in the northwestern Atlantic and transport variability of the cold Labrador Current. Understanding historic patterns of NAO variability requires long‐term and high‐resolution climate records that are not available from instrumental data. Here we present the first century‐scale proxy record of sea surface temperature (SST) variability from the Newfoundland shelf, a region from which other annual‐resolution shallow marine proxies are unavailable. The 116 year record was obtained from three sites along the eastern Newfoundland shelf using laser ablatio…

Atmospheric Science010504 meteorology & atmospheric sciencesSoil ScienceAquatic Science010502 geochemistry & geophysicsOceanography01 natural sciencesProxy (climate)Annual growth %Geochemistry and PetrologyClathromorphum compactumEarth and Planetary Sciences (miscellaneous)Marine ecosystem14. Life underwater0105 earth and related environmental sciencesEarth-Surface ProcessesWater Science and TechnologyEcologybiologyPaleontologyCoralline algaeForestrybiology.organism_classificationSea surface temperatureGeophysicsOceanography13. Climate actionSpace and Planetary ScienceNorth Atlantic oscillationClimatologyCrustoseGeology
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The evolution of microphysical and optical properties of an A380 contrail in the vortex phase

2012

A contrail from a large-body A380 aircraft at cruise in the humid upper troposphere has been probed with in-situ instruments onboard the DLR research aircraft Falcon. The contrail was sampled during 700 s measurement time at contrail ages of about 1–4 min. The contrail was in the vortex regime during which the primary wake vortices were sinking 270 m below the A380 flight level while the secondary wake remained above. Contrail properties were sampled separately in the primary wake at 90 and 115 s contrail age and nearly continously in the secondary wake at contrail ages from 70 s to 220 s. The scattering phase functions of the contrail particles were measured with a polar nephelometer. The …

Atmospheric Science010504 meteorology & atmospheric sciencesWakeAtmospheric sciences01 natural sciences010305 fluids & plasmaslcsh:ChemistryTroposphere0103 physical sciencesclimate impactWake turbulence0105 earth and related environmental sciences[SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereInstitut für Physik der AtmosphäreNephelometerIce crystalsAtmosphärische SpurenstoffeRadiative forcinglcsh:QC1-999FalconVortexlcsh:QD1-99913. Climate actionEnvironmental sciencePolarlcsh:Physics
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The Effect of the Covid-19 Lockdown on Air Quality in Three Italian Medium-Sized Cities

2020

Despite the societal and economic impacts of the COVID-19 pandemic, the lockdown measures put in place by the Italian government provided an unprecedented opportunity to increase our knowledge of the effect transportation and industry-related emissions have on the air quality in our cities. This study assessed the effect of reduced emissions during the lockdown period, due to COVID-19, on air quality in three Italian cities, Florence, Pisa, and Lucca. For this study, we compared the concentration of particulate matter PM10, PM2.5, NO2, and O3 measured during the lockdown period, with values obtained in the same period of 2019. Our results show no evidence of a direct relationship between th…

Atmospheric Science2019-20 coronavirus outbreakparticulate matter (PM)Coronavirus disease 2019 (COVID-19)nitrogen dioxideSevere acute respiratory syndrome coronavirus 2 (SARS-CoV-2)air pollutionCovid-19; lockdown; air pollution; particulate matter (PM); nitrogen dioxide; ozoneAir pollutionEnvironmental Science (miscellaneous)Particulateslcsh:QC851-999medicine.disease_causeAgricultural economicslockdownozonemedicineEnvironmental sciencelcsh:Meteorology. ClimatologyEconomic impact analysisHeavy trafficCovid-19Air quality index
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