Search results for "FLUX"

showing 10 items of 1392 documents

Annual pollen traps reveal the complexity of climatic control on pollen productivity in Europe and the Caucasus

2010

Annual PAR (pollen accumulation rates; grains cm−2 year−1) were studied with modified Tauber traps situated in ten regions, in Poland (Roztocze), the Czech Republic (two regions in Krkonoše, two in Šumava), Switzerland (4 regions in the Alps), and Georgia (Lagodekhi). The time-series are 10–16 years long, all ending in 2007. We calculated correlations between pollen data and climate. Pollen data are PAR summarized per region (4–7 traps selected per region) for each pollen type (9–14 per region) using log-transformed, detrended medians. Climate data are monthly temperature and precipitation measured at nearby stations, and their averages over all possible 2- to 6-month windows falling within…

570010506 paleontologyArcheology010504 meteorology & atmospheric sciencesEarth Sciences; Archaeology; Anthropology; Climate Change ; Biogeosciences; PaleontologyClimate changePlant Science580 Plants (Botany)medicine.disease_cause01 natural sciencesPollenmedicineAlnus viridisCyperaceae0105 earth and related environmental sciencesbiologyEcologyPalaeontologyPaleontology15. Life on landSeasonalitybiology.organism_classificationmedicine.diseaseGeographyProductivity (ecology)Pollen monitoring; Annual pollen accumulation; Influx; Climate; Europe; Caucasus13. Climate actionPhysical geographyLarchWoody plantVegetation History and Archaeobotany
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The intensity contrast of solar photospheric faculae and network elements : II. Evolution over the rising phase of solar cycle 23

2006

We studied the radiative properties of small magnetic elements (active region faculae and the network) during the rising phase of solar cycle 23 from 1996 to 2001, determining their contrasts as a function of heliocentric angle, magnetogram signal, and the solar cycle phase. We combined near-simultaneous full disk images of the line-of-sight magnetic field and photospheric continuum intensity provided by the MDI instrument on board the SOHO spacecraft. Sorting the magnetogram signal into different ranges allowed us to distinguish between the contrast of different magnetic structures. We find that the contrast center-to-limb variation (CLV) of these small magnetic elements is independent of …

:ASTRONOMÍA Y ASTROFÍSICA::Sistema solar [UNESCO]PlagesFOS: Physical sciencesSolar cycle 23AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAFaculaeMagnetogramSun activityRadiative transferAstrophysics::Solar and Stellar AstrophysicsPhysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Sistema solarSpacecraftbusiness.industryAstrophysics (astro-ph)SunContrast (statistics)Astronomy and AstrophysicsMagnetic fluxMagnetic fieldOn boardSun activity ; Faculae ; Plages ; Sun ; Magnetic fieldsSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsAstrophysics::Earth and Planetary Astrophysicsbusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

2009

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming ντ may interact in the Earth's crust and produce a τ lepton by means of charged-current interactions. The τ lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by τ decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is de…

ACTIVE GALACTIC NUCLEIASTROPHYSICS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsActive galactic nucleusPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayPROPAGATIONAstrophysics7. Clean energy01 natural sciencesLeptonSpectral lineSettore FIS/04 - Fisica Nucleare e SubnucleareAugerSEARCHTau neutrino0103 physical sciencesTau neutrinoOSCILLATIONS010306 general physicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSPierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaultrahigh energy cosmic rays ; tau neutrinos ; Pierre Auger ObservatoryDiffuse fluxPierre Auger ObservatoryPERFORMANCECOSMIC-RAYScosmic radiation13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaLeptonPhysical Review D
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Measurement of the AtmosphericνeSpectrum with IceCube

2015

We present a measurement of the atmospheric $\nu_e$ spectrum at energies between 0.1 TeV and 100 TeV using data from the first year of the complete IceCube detector. Atmospheric $\nu_e$ originate mainly from the decays of kaons produced in cosmic-ray air showers. This analysis selects 1078 fully contained events in 332 days of livetime, then identifies those consistent with particle showers. A likelihood analysis with improved event selection extends our previous measurement of the conventional $\nu_e$ fluxes to higher energies. The data constrain the conventional $\nu_e$ flux to be $1.3^{+0.4}_{-0.3}$ times a baseline prediction from a Honda's calculation, including the knee of the cosmic-…

AMANDANuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaHadronCASCADES01 natural sciences7. Clean energyPower lawIceCubeNuclear physicsFlux (metallurgy)DESIGNLikelihood analysisDIGITIZATION0103 physical sciencesNEUTRINO FLUX010306 general physicsDETECTORPhysics010308 nuclear & particles physicsICEHigh Energy Physics::PhenomenologySpectrum (functional analysis)DetectorPERFORMANCEENERGY-SPECTRUMEvent selectionPhysics and AstronomyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsSYSTEMPhysical Review D
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Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

2003

We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

AMANDAcosmic radiation [neutrino]Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]General Physics and AstronomyFOS: Physical sciencesAstrophysicsmagnetic [matter]Astrophysicsnumerical methodsddc:550quasarBlazarAstroparticle physicsPhysicsphotomultipliercosmic radiation [muon]water [Cherenkov counter]Astrophysics (astro-ph)AstronomySolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentflux [cosmic radiation]blazar [AGN]data managementNeutrinoupper limitexperimental results
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Are remote sensing evapotranspiration models reliable across South American ecoregions?

2021

Many remote sensing-based evapotranspiration (RSBET) algorithms have been proposed in the past decades and evaluated using flux tower data, mainly over North America and Europe. Model evaluation across South America has been done locally or using only a single algorithm at a time. Here, we provide the first evaluation of multiple RSBET models, at a daily scale, across a wide variety of biomes, climate zones, and land uses in South America. We used meteorological data from 25 flux towers to force four RSBET models: Priestley–Taylor Jet Propulsion Laboratory (PT-JPL), Global Land Evaporation Amsterdam Model (GLEAM), Penman–Monteith Mu model (PM-MOD), and Penman–Monteith Nagler model (PME-VI).…

ATMOSPHERE WATER FLUXVEGETATION INDEXCalibration (statistics)Penman-MonteithBiomeRIPARIAN EVAPOTRANSPIRATIONFluxLand coverSURFACE-TEMPERATUREtranspirationSEMIARID ENVIRONMENTCARBON-DIOXIDEENERGY-BALANCE CLOSUREEvapotranspirationPenman–Monteith equationWater Science and TechnologyRemote sensingRAINFALL INTERCEPTIONLand useWACMOS-ET PROJECTEDDY COVARIANCE MEASUREMENTSMODISEarth and Environmental SciencesEnvironmental sciencePriestley-TaylorScale (map)
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Isopetasin and S-isopetasin as novel P-glycoprotein inhibitors against multidrug-resistant cancer cells

2019

Abstract Background A major problem of cancer treatment is the development of multidrug resistance (MDR) to chemotherapy. MDR is caused by different mechanisms such as the expression of the ABC-transporters P-glycoprotein (P-gp, MDR1, ABCB1) and breast cancer resistance protein (BCRP, ABCG2). These transporters efflux xenobiotic toxins, including chemotherapeutics, and they were found to be overexpressed in different cancer types. Purpose Identification of novel molecules that overcome MDR by targeting ABC-transporters. Methods Resazurin reduction assay was used for cytotoxicity test. AutoDock 4.2. was used for molecular docking. The function of P-gp and BCRP was tested using a doxorubicin …

ATP Binding Cassette Transporter Subfamily BAbcg2Pharmaceutical Science03 medical and health sciences0302 clinical medicineCell Line TumorDrug DiscoverymedicineHumansCytotoxic T cell030304 developmental biologyP-glycoproteinPharmacology0303 health sciencesbiologyChemistryCancermedicine.diseaseDrug Resistance MultipleNeoplasm ProteinsMolecular Docking SimulationMultiple drug resistanceComplementary and alternative medicineDrug Resistance NeoplasmApoptosis030220 oncology & carcinogenesisCancer cellbiology.proteinCancer researchMolecular MedicineEffluxSesquiterpenesPhytomedicine
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Psychometric validation of the Italian translation of the gastrointestinal symptom-rating scale and quality of life in reflux and dyspepsia questionn…

2007

Background: Symptoms of heartburn and their impact on health-related quality of life (HR-QOL) are often evaluated in clinical trials. When a questionnaire is translated into a new language, a linguistic validation is necessary but not sufficient unless the psychometric characteristics have been verified. Objective: To document the psychometric characteristics of the Italian translation of the Gastrointestinal Symptom-Rating Scale (GSRS) and Quality of Life in Reflux and Dyspepsia (QOLRAD) questionnaire. Patients and methods: 152 consecutive patients with symptoms of heartburn (mean ±SD age 46.5 ± 16.2 years; 40.1% males) completed the Italian translation of GSRS, the heartburn version of QO…

Abdominal painmedicine.medical_specialtyGASTROINTESTINAL SYMPTOM-RATING SCALEPSYCHOMETRIC VALIDATIONREFLUX AND DYSPEPSIAbusiness.industryRefluxHeartburnGeneral MedicineGERDLinguistic validationmedicine.diseaseIndigestionQuality of lifeQUALITY OF LIFERating scaleGERDPhysical therapyMedicinePharmacology (medical)medicine.symptombusiness
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Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign

2021

Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; …

Accretion010504 meteorology & atmospheric sciencesAstronomyFluxAstrophysics7. Clean energy01 natural sciencesActive galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; Accretion; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HERadio coreAccretion (meteorology)PhysicsAstrophysical black holes520 Astronomie und zugeordnete WissenschaftenActive galactic nuclei ; Radio cores ; Low-luminosity ; active galactic nuclei ; High energy astrophysics ; Astrophysical black holes ; AccretionAstrophysical black holeLow-luminosity active galactic nucleiastro-ph.COAstrophysics - High Energy Astrophysical PhenomenaAccretion; Active galactic nuclei; Astrophysical black holes; High energy astrophysics; Low-luminosity active galactic nuclei; Radio coresHigh energy astrophysicsRadio coresAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusHigh-energy astronomyastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesF500Astrophysics::Cosmology and Extragalactic AstrophysicsHigh energy astrophysic0103 physical sciencesVery-long-baseline interferometryddc:530Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeActive galactic nucleiAstronomy and Astrophysics530 PhysikAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ddc:520Active galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; AccretionHESS - Abteilung Hinton[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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A Hard X-Ray View of Scorpius X-1 with INTEGRAL : Nonthermal Emission?

2006

We present here simultaneous INTEGRAL/RXTE observations of Sco X-1, and in particular a study of the hard X-ray emission of the source and its correlation with the position in the Z-track of the X-ray color-color diagram. We find that the hard X-ray (above about 30 keV) emission of Sco X-1 is dominated by a power-law component with a photon index of ~3. The flux in the power-law component slightly decreases when the source moves in the color-color diagram in the sense of increasing inferred mass accretion rate from the horizontal branch to the normal branch/flaring branch vertex. It becomes not significantly detectable in the flaring branch, where its flux has decreased by about an order of…

AccretionPhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciencesneutron starsX-ray[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Position (vector)Accretion DisksStars: Neutron0103 physical sciencesX-Rays: StarsAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)DiagramAstronomy and AstrophysicsSense (electronics)Horizontal branchX-Rays: BinariesX-Rays: GeneralSpace and Planetary ScienceVertex (curve)accreting millisecondStars: Individual: Constellation Name: Scorpius X-1Order of magnitudeThe Astrophysical Journal
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