Search results for "instrument"

showing 10 items of 5652 documents

A Search for IceCube Events in the Direction of ANITA Neutrino Candidates

2020

During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy up-going air shower and compatible with a tau neutrino interpretation. A third neutrino candidate event was detected in a search for Askaryan radiation in the Antarctic ice, although it is also consistent with the background expectation. The inferred emergence angle of the first two events is in tension with IceCube and ANITA limits on isotropic cosmogenic neutrino fluxes. Here, we test the hypothesis that these events are astrophysical in origin, possibly caused by a po…

010504 meteorology & atmospheric sciencesPoint sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Tau neutrino0103 physical sciencesTRACK RECONSTRUCTIONSource spectrum010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEIsotropyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicshep-phHigh Energy Physics - PhenomenologyAir showerPhysics and Astronomy13. Climate actionSpace and Planetary ScienceNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)
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Validation of a novel Multi-Gas sensor for volcanic HCl alongside H2S and SO2 at Mt. Etna

2017

Erratum to: Bull Volcanol (2017) 79: 36DOI 10.1007/s00445-017-1114-zDuring the steps of corrections, the publisher inadvertently changed the author affiliations so that they were no longer correct. The correct information is given below. The publisher regrets this mistake.; International audience; Volcanic gas emission measurements inform predictions of hazard and atmospheric impacts. For these measurements, Multi-Gas sensors provide low-cost in situ monitoring of gas composition but to date have lacked the ability to detect halogens. Here, two Multi-Gas instruments characterized passive outgassing emissions from Mt. Etna’s (Italy) three summit craters, Voragine (VOR), North-east Crater (NE…

010504 meteorology & atmospheric sciencesResponse modelPoison controlMineralogyOpen-system volcanic degassing010502 geochemistry & geophysics01 natural sciencesElectronic noseImpact craterGeochemistry and PetrologyCalibrationGas compositionVolcanic outgassing0105 earth and related environmental sciencesMulti-Gas instrumentgeographygeography.geographical_feature_categoryE-noseOutgassingVolcano13. Climate action[SDU]Sciences of the Universe [physics]HalogenMagmaChlorineGeology
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Evidence of active fluid seepage (AFS) in the southern region of the central Mediterranean Sea

2018

Abstract Active fluid seepage (AFS) at the seafloor is a global phenomenon associated with seafloor morphologies in different geodynamic contexts. Advanced geophysical techniques have allowed geoscientists to characterise pockmarks, mounds and flares associated with AFS. We present a range of new marine geological data acquired in the southern region of the central Mediterranean Sea (northern Sicily continental margin, northwestern Sicily Channel and offshore of the Maltese Islands), which allow us to identify AFSs. AFSs are spatially distributed as clusters, aligned or isolated at different depths, ranging from few decametres offshore of the Maltese Islands; up to 400 m offshore of norther…

010504 meteorology & atmospheric sciencesSicily ChannelSettore GEO/02 - Geologia Stratigrafica E SedimentologicaRange (biology)Settore GEO/03 - Geologia Strutturale010502 geochemistry & geophysics01 natural sciencesFluid seepagePaleontologyGas flaresMediterranean seaContinental marginElectrical and Electronic EngineeringInstrumentation0105 earth and related environmental sciencesMoundgeographyFluid seepage; Gas flares; Mound; Pockmark; Sicily Channel; Instrumentation; Electrical and Electronic Engineeringgeography.geographical_feature_categoryContinental shelfApplied MathematicsPockmarkFluid seepage; Gas flares; Mound; Pockmark; Sicily ChannelGas flareCondensed Matter PhysicsSeafloor spreadingPockmarkSubmarine pipelineGeologyChannel (geography)
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Observation of classically 'forbidden' electromagnetic wave propagation and implications for neutrino detection.

2018

Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in-ice or in-air, is used to infer the properties of the neutrino. To evaluate their experimental sensitivity, such experiments require a refractive index model for ray tracing radio-wave trajectories from a putative in-ice neutrino interaction point to the receiving antennas; this gives the degree of signal absorption or ray bending from source to receiver. The gradient in the density profile over the upper 200 meters of Antarctic ice, coupled wi…

010504 meteorology & atmospheric sciencesWave propagationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesElectromagnetic radiationAtomicIce shelfParticle and Plasma Physics0103 physical sciencesddc:530NuclearInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics::Atmospheric and Oceanic Physics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)geographygeography.geographical_feature_categoryultra high energy photons and neutrinos010308 nuclear & particles physicsMolecularAstronomy and AstrophysicsNuclear & Particles PhysicsComputational physicsRay tracing (physics)Radio propagationNeutrino detectorcosmic ray experimentsNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstronomical and Space SciencesRadio wave
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First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

2019

We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μas, with characteristic sensitivity limits of ~1 mJy on baselines to ALMA and ~10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, …

010504 meteorology & atmospheric sciencesgalaxies: jetRadio galaxyAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies: individualGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgalaxies: individual: M8701 natural sciencesSubmillimeter ArrayGeneral Relativity and Quantum CosmologyTechniques: high angular resolutionindividual (M87 3C279) [Galaxies]0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics0105 earth and related environmental sciencesRemote sensingPhysicsEvent Horizon TelescopeSupermassive black hole3C279Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasarBlack hole physicsblack hole physicAstrophysics - Astrophysics of Galaxies3. Good healthhigh angular resolution [Techniques]InterferometryAmplitudeSpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]jets [Galaxies]Astrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Galaxies: individual (M87 3C279)Radio wave
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First M87 Event Horizon Telescope Results. II. Array and Instrumentation

2019

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ~1.3 mm, EHT angular resolution (λ/D) is ~25 μas, which is sufficient to resolve nearby supermassive black hole candidates on spatial and temporal scales that correspond to their event horizons. With this capability, the EHT scientific goals are to probe general relativistic effects in the strong-field regime and to study accretion and relativistic jet formation near the black hole boundary. In this Letter we describe the system design of th…

010504 meteorology & atmospheric sciencesindividual (M87) [galaxies]Event horizonAstronomyAstrophysics::High Energy Astrophysical Phenomenainterferometers [instrumentation]black hole physicsFOS: Physical sciencesgalaxies: individualGeneral Relativity and Quantum Cosmology (gr-qc)galaxies: individual: M8701 natural sciencesGeneral Relativity and Quantum Cosmologygalaxies: individual (M87)instrumentation: interferometer0103 physical sciencesVery-long-baseline interferometryAngular resolutionInstrumentation (computer programming)instrumentation: interferometers010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy Astrophysics0105 earth and related environmental scienceshigh angular resolution [echniques]Event Horizon TelescopePhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Supermassive black holeGalaxy: centerhigh angular resolution [techniques]Astronomytechniques: high angular resolutiongravitational lensing: strongAstronomy and Astrophysicscenter [Galaxy]Hydrogen maserblack hole physicAstrophysics - Astrophysics of Galaxiesechniques: high angular resolutionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)strong [gravitational lensing]MillimeterAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]The Astrophysical Journal Letters
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Characterization of a Newly Developed Aircraft-Based Laser Ablation Aerosol Mass Spectrometer (ALABAMA) and First Field Deployment in Urban Pollution…

2011

We present here the development and first field deployment of a novel Aircraft-based Laser ABlation Aerosol MAss spectrometer (ALABAMA), which is capable of measuring the chemical composition and size of individual ambient aerosol particles in the size range between 150 and 900 nm. The instrument uses a continuous wave 532 nm laser to size and detect the particles, a pulsed 266 nm laser to ablate and ionize the particles, and a bipolar, Z-shaped time-of-flight mass spectrometer to detect positive and negative ions. The ALABAMA fits into a 19"-aircraft rack of 150 cm height and has a total weight of 140 kg, thus currently being one of the smallest and lightest-weight instruments of its type.…

010504 meteorology & atmospheric sciencesinstrument developmentaerosolMineralogy01 natural scienceslaw.inventionOpticslawparticle composition11. SustainabilityEnvironmental ChemistryGeneral Materials ScienceParticle beam0105 earth and related environmental sciencesRange (particle radiation)Laser ablationbusiness.industryChemistry010401 analytical chemistryAtmosphärische SpurenstoffeLaserPollution0104 chemical sciencesAerosol13. Climate actionMass spectrumParticleParticle sizeAerosol Mass spectrometerbusinessAerosol Science and Technology
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Time domain astronomy with the THESEUS satellite

2021

THESEUS is a medium size space mission of the European Space Agency, currently under evaluation for a possible launch in 2032. Its main objectives are to investigate the early Universe through the observation of gamma-ray bursts and to study the gravitational waves electromagnetic counterparts and neutrino events. On the other hand, its instruments, which include a wide field of view X-ray (0.3-5 keV) telescope based on lobster-eye focussing optics and a gamma-ray spectrometer with imaging capabilities in the 2-150 keV range, are also ideal for carrying out unprecedented studies in time domain astrophysics. In addition, the presence onboard of a 70 cm near infrared telescope will allow simu…

010504 meteorology & atmospheric sciencesmedia_common.quotation_subjectAstronomyAstrophysics::High Energy Astrophysical PhenomenaSocio-culturaleFOS: Physical sciencesX-ray sources01 natural scienceslaw.inventionTelescopeX-ray sourceSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesTime domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Variability010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesmedia_commonTime domain astronomyPhysicsSpectrometerGravitational waveX-rays surveysAstronomyAstronomy and AstrophysicsUniverseSpace and Planetary ScienceSatelliteNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsExperimental Astronomy
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First in-situ measurements of plume chemistry at mount garet volcano, island of gaua (Vanuatu)

2020

Recent volcanic gas compilations have urged the need to expand in-situ plume measurements to poorly studied, remote volcanic regions. Despite being recognized as one of the main volcanic epicenters on the planet, the Vanuatu arc remains poorly characterized for its subaerial emissions and their chemical imprints. Here, we report on the first plume chemistry data for Mount Garet, on the island of Gaua, one of the few persistent volatile emitters along the Vanuatu arc. Data were collected with a multi-component gas analyzer system (multi-GAS) during a field campaign in December 2018. The average volcanic gas chemistry is characterized by mean molar CO2/SO2, H2O/SO2, H2S/SO2 and H2/SO2 ratios …

010504 meteorology & atmospheric sciencesvolcanic gas compositionsGeochemistryFlux010502 geochemistry & geophysicslcsh:Technology01 natural scienceslcsh:ChemistryVanuatu[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologyGeneral Materials ScienceGas composition[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentlcsh:QH301-705.5Instrumentation0105 earth and related environmental sciencesFluid Flow and Transfer Processesgeographygeography.geographical_feature_categorySubductionlcsh:TProcess Chemistry and TechnologyGeneral Engineeringlcsh:QC1-999Gas analyzerComputer Science ApplicationsPlumelcsh:Biology (General)lcsh:QD1-999Mount GaretVolcanolcsh:TA1-2040SubaerialPeriod (geology)volatile fluxeslcsh:Engineering (General). Civil engineering (General)GauaGaua Mount Garet Multi-GAS Vanuatu Volatile fluxes Volcanic gas compositionslcsh:PhysicsMulti-GAS
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Highly-resolved radiocarbon measurements on shells from Kalba, UAE, using carbonate handling system and gas ion source with MICADAS

2019

Abstract The Mini Carbon Dating System (MICADAS) represents a flexible AMS system for measuring radiocarbon samples either in the form of graphite or CO2 gas. We used the possibility to attach a carbonate handling system (CHS) to the gas ion source (GIS) to measure smaller amounts of carbonates (  3) are used to clean the system. We tested the CHS-GIS combination on heated and unheated archaeological shells of Anadara uropigimelana from Kalba, Sharjah Emirate, United Arab Emirates (UAE). Even though the amount of carbon in the samples was small (4–22 µg C) the performance of the CO2 dating system permits the comparison of trends in the 14C data to stable isotope measurements (δ18O and δ13C)…

010506 paleontologyNuclear and High Energy Physicsδ18OStable isotope ratiochemistry.chemical_elementMineralogy010502 geochemistry & geophysics01 natural sciencesIon sourcelaw.inventionHandling systemchemistry.chemical_compoundchemistrylawCarbonateEnvironmental scienceRadiocarbon datingGraphiteInstrumentationCarbon0105 earth and related environmental sciencesNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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