Search results for "Lag"

showing 10 items of 3124 documents

Dental calculus is not equivalent to bone collagen for isotope analysis: a comparison between carbon and nitrogen stable isotope analysis of bulk den…

2014

Palaeodietary reconstruction using the carbon and nitrogen isotope values of bone and dentine collagen is a well-established method and the biochemical processes involved are well known. Researchers have recently explored using bulk samples of dental calculus as a substitute for bone and dentine collagen in dietary analyses, because calculus can be sampled without causing damage to the teeth, and may be useful in situations where more destructive analyses are not possible, or where collagen is poorly preserved. Several questions remain about the use of bulk calculus as a source of carbon and nitrogen isotope data, however. It is not yet clear how much of an individual¿s life span dental cal…

Arqueologia medievalArcheologyBone collagenIsotopeChemistryStable isotope ratioCalculus (dental)educationMineralogychemistry.chemical_elementmedicine.diseaseNitrogenIsotopes of nitrogenstomatognathic diseasesmedicineCalculusCarbonIsotope analysisJournal of Archaeological Science
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COMMENTO AGLI ARTT. 379,380,381,382,383 c.p.p.

2012

Arrestoflagranza reato
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Horse exploitation at the Late Upper Palaeolithic site of Oelknitz (Thuringia, Germany) with special reference to canine modifications

2012

Abstract The faunal assemblage from Structure 5 of the Magdalenian settlement Oelknitz (Thuringia, Germany) was analyzed. The fauna is dominated by horse. All stages of butchery from skinning to marrow extraction were performed within the horse assemblage. In addition to this, various stages of organic artifact production could be documented. Two fragmentary equid canine teeth were of particular interest. They are the only documented canines from Structure 5, which otherwise contained a large amount of teeth. Both canines show traces of human modification. They were cut out of the jaw while still in the alveole. On both canines, lateral incisions were performed at the cervix dentis and the …

Artifact (archaeology)FaunaTooth enamelArchaeologyAntlerstomatognathic diseasesGeographymedicine.anatomical_structurestomatognathic systemmedicineAssemblage (archaeology)CarnivoreMagdalenianEarth-Surface ProcessesFaunal assemblageQuaternary International
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Présence d’Asellides stygobies (Crustacea, Isopoda, Aselloidea) dans la région du Primorye, Sibérie sud-orientale

1993

Two species of anophthalmous, unpigmentedasellids have been found in springs and groundwaters of S.E. Siberia (Primorye region). Asellus (Asellus) primoryensis n. sp. is closelyrelated to the epigean species A. (A.) hilgendorfii Bovallius, 1886, as is the case for all stygobiont Asellus (Asellus) species previously known from the Japanese archipelago. Sibirasellus parpurae n. g., n. sp. is closely related to the microphthalmous species Asellus dentifer Birstein & Levanidov, 1952 from the Ussuri Basin (Khor region), now type-species of the new genus Sibirasellus. These two species show several original characters: body covered by numerous cuticular squamulae, mandibular palp reduced (gla…

Asellusgeographygeography.geographical_feature_categoryEcologymedia_common.quotation_subjectBiogeographyBiologybiology.organism_classificationstygobiont asellidsCoalescent theorytaxonomyFar East and Pacific North AmericaGenusArchipelagoGeneral Earth and Planetary SciencesTaxonomy (biology)SubgenusPhyletic gradualismbiogeographyGeneral Environmental Sciencemedia_common
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OBSERVATION OF THE TeV GAMMA-RAY SOURCE MGRO J1908+06 WITH ARGO-YBJ

2012

The extended gamma ray source MGRO J1908+06, discovered by the Milagro air shower detector in 2007, has been observed for about 4 years by the ARGO-YBJ experiment at TeV energies, with a statistical significance of 6.2 standard deviations. The peak of the signal is found at a position consistent with the pulsar PSR J1907+0602. Parametrizing the source shape with a two-dimensional Gauss function we estimate an extension \sigma = 0.49 \pm 0.22 degrees, consistent with a previous measurement by the Cherenkov Array H.E.S.S.. The observed energy spectrum is dN/dE = 6.1 \pm 1.4 \times 10^-13 (E/4 TeV)^{-2.54 \pm 0.36} photons cm^-2 s^-1 TeV^-1, in the energy range 1-20 TeV. The measured gamma ray…

Astrophysics::High Energy Astrophysical PhenomenaAstrophysicsgeneral – pulsars: individual (MGRO J1908+06) [gamma rays]7. Clean energy01 natural sciencesPulsar wind nebulaLuminositySettore FIS/05 - Astronomia E AstrofisicaPulsar0103 physical sciences010303 astronomy & astrophysicspulsarPhysics010308 nuclear & particles physicsgamma rays: general – pulsars: individual (MGRO J1908+06)Settore FIS/01 - Fisica SperimentaleGamma rayAstronomy and Astrophysics(MGRO J1908+06)Air showerCrab Nebula13. Climate actionSpace and Planetary Sciencegamma rayMilagroHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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Updating the orbital ephemeris of the dipping source XB 1254-690 and the distance to the source

2017

XB 1254-690 is a dipping low mass X-ray binary system hosting a neutron star and showing type I X-ray bursts. We aim at obtaining more accurate orbital ephemeris and at constraining the orbital period derivative of the system for the first time. In addition, we want to better constrain the distance to the source in order to locate the system in a well defined evolutive scenario. We apply for the first time an orbital timing technique to XB 1254-690, using the arrival times of the dips present in the light curves that have been collected during 26 years of X-ray pointed observations performed from different space missions. We estimate the dip arrival times using a statistical method that wei…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLagrangian pointAstrophysicsStar (graph theory)Ephemeris01 natural sciencesstars: neutron0103 physical sciencesX-rays: star010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsstars: individual (XB 1254690)Astronomy and AstrophysicsQuadratic functionAstronomy and AstrophysicOrbital periodLight curveX-rays: binarieAstrometry and celestial mechanics: ephemerideNeutron starSpace and Planetary Scienceephemerides; stars: individual (XB 1254690); stars: neutron; X-rays: binaries; X-rays: stars; Astronomy and Astrophysics; Space and Planetary Science [Astrometry and celestial mechanics]Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLow Mass
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Observation of TeV gamma rays from the Cygnus region with the ARGO-YBJ experiment

2012

We report the observation of TeV gamma-rays from the Cygnus region using the ARGO-YBJ data collected from 2007 November to 2011 August. Several TeV sources are located in this region including the two bright extended MGRO J2019+37 and MGRO J2031+41. According to the Milagro data set, at 20 TeV MGRO J2019+37 is the most significant source apart from the Crab Nebula. No signal from MGRO J2019+37 is detected by the ARGO-YBJ experiment, and the derived flux upper limits at 90% confidence level for all the events above 600 GeV with medium energy of 3 TeV are lower than the Milagro flux, implying that the source might be variable and hard to be identified as a pulsar wind nebula. The only statist…

Astrophysics::High Energy Astrophysical Phenomenageneral – pulsars: individual (MGRO J2019+37 [Gamma rays]FluxFOS: Physical sciencesAstrophysics01 natural sciencesPulsar wind nebulageneral – pulsar0103 physical sciencesMILAGRO010303 astronomy & astrophysicsDETECTORArgoPhysicsCALIBRATIONHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsMGRO J2031+41)Settore FIS/01 - Fisica SperimentaleGamma rayAstronomy and Astrophysicsindividual (MGRO J2019+37 MGRO J2031+41)PLANE3. Good healthMedium energyCrab Nebulagamma ray13. Climate actionSpace and Planetary ScienceGALACTIC SOURCESJ2032+4130Milagrogamma rays; general – pulsars; individual (MGRO J2019+37 MGRO J2031+41)EMISSIONAstrophysics - High Energy Astrophysical Phenomena
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The stereographic coordinate system

2003

Atmospheresymbols.namesakeClassical mechanicsCoordinate systemDynamics (mechanics)Image scalesymbolsEquations of motionStereographic projectionConformal mapGeometryLagrangianMathematics
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Lagrangian Description of Air Masses Associated with Latent Heat Release in Tropical Storm Karl (2016) during Extratropical Transition

2019

Abstract Extratropical transition (ET) of tropical cyclones involves distinct changes of the cyclone’s structure that are not yet well understood. This study presents for the first time a comprehensive Lagrangian description of structure change near the inner core. A large sample of trajectories is computed from a convection-permitting numerical simulation of the ET of Tropical Storm Karl (2016). Three main airstreams are considered: those associated with the inner-core convection, inner-core descent, and the developing warm conveyor belt. Analysis of these airstreams is performed both in thermodynamic and physical space. Prior to ET, Karl is embedded in weak vertical wind shear and its int…

Atmospheric Science010504 meteorology & atmospheric sciencesAirflow020207 software engineering02 engineering and technology01 natural sciencesDeep convectionsymbols.namesakeClimatologyLatent heat0202 electrical engineering electronic engineering information engineeringExtratropical cyclonesymbolsEnvironmental scienceCycloneTropical cycloneLagrangian0105 earth and related environmental sciencesMonthly Weather Review
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Ground-based off-line aerosol measurements at Praia, Cape Verde, during the Saharan Mineral Dust Experiment: microphysical properties and mineralogy

2011

A large field experiment of the Saharan Mineral Dust Experiment (SAMUM) was performed in Praia, Cape Verde, in January and February 2008. This work reports on the aerosol mass concentrations, size distributions and mineralogical composition of the aerosol arriving at Praia. Three dust periods were recorded during the measurements, divided by transitional periods and embedded in maritime-influenced situations. The total suspended particle mass/PM 10 /PM 2.5 were 250/180/74 μg/m 3 on average for the first dust period (17–21 January) and 250/230/83 μg/m 3 for the second (24–26 January). The third period (28 January to 2 February) was the most intensive with 410/340/130 μg/m 3 . Four modes were…

Atmospheric Science010504 meteorology & atmospheric sciencesMineralogy010501 environmental sciencesengineering.materialMineral dust01 natural sciencesAerosolCape verdedust ; aerosol ; clay particles ; microphysical propertiesIlliteengineeringEnvironmental sciencePlagioclaseKaoliniteHaliteQuartz0105 earth and related environmental sciencesTellus B
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