Search results for "nuclei"

showing 10 items of 1273 documents

A Highly Magnetized Twin-Jet Base Pinpoints a Supermassive Black Hole

2016

Supermassive black holes (SMBH) are essential for the production of jets in radio-loud active galactic nuclei (AGN). Theoretical models based on Blandford & Znajek extract the rotational energy from a Kerr black hole, which could be the case for NGC1052, to launch these jets. This requires magnetic fields of the order of $10^3\,$G to $10^4\,$G. We imaged the vicinity of the SMBH of the AGN NGC1052 with the Global Millimetre VLBI Array and found a bright and compact central feature, smaller than 1.9 light days (100 Schwarzschild radii) in radius. Interpreting this as a blend of the unresolved jet bases, we derive the magnetic field at 1 Schwarzschild radius to lie between 200 G and ~8000…

AstrofísicaCamps magnèticsActive galactic nucleus[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsmagnetic fields01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSupermassive black holeJet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsRadiusgalaxies: jetsAstrophysics - Astrophysics of GalaxiesMagnetic fieldRotational energyRotating black holeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstronomiagalaxies: nucleiAstrophysics - High Energy Astrophysical Phenomenagalaxies: magnetic fields[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Schwarzschild radius
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SEARCH FOR A CORRELATION BETWEEN ANTARES NEUTRINOS AND PIERRE AUGER OBSERVATORY UHECRs ARRIVAL DIRECTIONS

2013

A multimessenger analysis optimized for a correlation of arrival directions of ultra-high energy cosmic rays (UHECRs) and neutrinos is presented and applied to 2190 neutrino candidate events detected in 2007-2008 by the ANTARES telescope and 69 UHECRs observed by the Pierre Auger Observatory between 2004 January 1 and 2009 December 31. No significant correlation is observed. Assuming an equal neutrino flux (E-2 energy spectrum) from all UHECR directions, a 90% CL upper limit on the neutrino flux of 5.0 x 10(-8) GeV cm(-2) s(-1) per source is derived.

AstrofísicaSELECTIONPOINT SOURCESTELESCOPE[PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]Astrophysics::High Energy Astrophysical Phenomenaastroparticle physics – cosmic rays – neutrinos[SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP]FOS: Physical sciencesCosmic rayAstrophysicsPROPAGATIONACCELERATION7. Clean energy01 natural scienceslaw.inventionTelescopecosmic rayslaw0103 physical sciencesICECUBE DETECTORBURSTSNeutrinos010303 astronomy & astrophysicsCosmic raysPierre Auger ObservatoryAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NUCLEI010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrinosastroparticle physicAstronomy and AstrophysicsGALACTIC MAGNETIC-FIELDMassless particleENERGY COSMIC-RAYSSpace and Planetary Scienceastroparticle physicsFISICA APLICADAHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)Lepton
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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

2010

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating…

AstronomyAstrophysicsUltra High Energy Cosmic ray01 natural scienceslaw.inventionObservatorylawAnisotropy010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]UHECRAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKAnisotropíaGALAXIESNEUTRINOSGreisen–Zatsepin–Kuz’minComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEIHIPASS CATALOG[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleusRadiación Cósmicamedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsTelescope0103 physical sciencesCosmic raysCiencias ExactasAstrophysics::Galaxy AstrophysicsPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsAstronomyFísicaAstronomy and AstrophysicsCosmic rayGalaxyCorrelation with astrophysical sourcesCosmic rays; UHECR; Anisotropy; Pierre Auger Observatory; Extra-galactic; GZKSkyExperimental High Energy PhysicsAnisotropyExtra-galactic
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The frontiers of the virtual photons program at MAMI

2012

The most recent results and the future physics program of the high precision electron-scattering experiment at MAMI are briefly outlined. The A1 high-resolution spectrometers facility allows for a unique quality of virtual photon experiments. High precision form factor measurements, few-baryon systems highresolution structure studies and the innovative way in the search of dark photons illustrate the interplay between such diverse fields as precision atomic physics, nuclear astrophysics and astroparticle physics, where hadron physics plays a central and connecting role.

Astroparticle physicsPhysicsParticle physicsPhotonSpectrometerPhysicsQC1-999Form factor (quantum field theory)Virtual particleEngineering physicsHadron physicsNuclear astrophysicsvirtual photon; form factor measurements; dark photon; precision spectroscopy of light hypernucleiNuclear Experiment
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Primary biological aerosol particles in the atmosphere: a review

2012

Atmospheric aerosol particles of biological origin are a very diverse group of biological materials and structures, including microorganisms, dispersal units, fragments and excretions of biological organisms. In recent years, the impact of biological aerosol particles on atmospheric processes has been studied with increasing intensity, and a wealth of new information and insights has been gained. This review outlines the current knowledge on major categories of primary biological aerosol particles (PBAP): bacteria and archaea, fungal spores and fragments, pollen, viruses, algae and cyanobacteria, biological crusts and lichens and others like plant or animal fragments and detritus. We give a…

AtmosphereAtmospheric ScienceDetritusPrimary (chemistry)MicroorganismIce nucleusCloud condensation nucleiAtmospheric sciencesLichenAerosolTellus B: Chemical and Physical Meteorology
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African volcanic emissions influencing atmospheric aerosols over the Amazon rain forest

2018

Long-range transport (LRT) plays an important role in the Amazon rain forest by bringing in different primary and secondary aerosol particles from distant sources. The atmospheric oxidation of dimethyl sulfide (DMS), emitted from marine plankton, is considered an important sulfate source over the Amazon rain forest, with a lesser contribution from terrestrial soil and vegetation sulfur emissions. Volcanic sulfur emissions from Africa could be a source of particulate sulfate to the Amazonian atmosphere upon transatlantic transport but no observations have been published. By using satellite observations, together with ground‑based and airborne aerosol particle observations, this paper provide…

Atmospheric Science010504 meteorology & atmospheric sciencesAmazonian[SDE.MCG]Environmental Sciences/Global Changes010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencescomplex mixtureslcsh:ChemistryAtmospherechemistry.chemical_compoundparasitic diseasesCloud condensation nucleiSulfate0105 earth and related environmental sciences[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmospheregeographygeography.geographical_feature_category15. Life on landParticulateslcsh:QC1-999Trace gasAerosollcsh:QD1-999Volcanochemistry13. Climate actionEnvironmental sciencegeographic locationslcsh:Physics
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2016

Abstract. Cloud residues and out-of-cloud aerosol particles with diameters between 150 and 900 nm were analysed by online single particle aerosol mass spectrometry during the 6-week study Hill Cap Cloud Thuringia (HCCT)-2010 in September–October 2010. The measurement location was the mountain Schmücke (937 m a.s.l.) in central Germany. More than 160 000 bipolar mass spectra from out-of-cloud aerosol particles and more than 13 000 bipolar mass spectra from cloud residual particles were obtained and were classified using a fuzzy c-means clustering algorithm. Analysis of the uncertainty of the sorting algorithm was conducted on a subset of the data by comparing the clustering output with parti…

Atmospheric Science010504 meteorology & atmospheric sciencesChemistryMineralogy010501 environmental sciencesAtmospheric sciencesmedicine.disease_causecomplex mixtures01 natural sciencesSootAerosolchemistry.chemical_compoundLiquid water contentmedicineCloud condensation nucleiParticleAerosol mass spectrometrysense organsSulfateSea salt aerosol0105 earth and related environmental sciencesAtmospheric Chemistry and Physics
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Aerosol influences on low-level clouds in the West African monsoon

2019

Abstract. Low-level clouds (LLC) cover a wide area of southern West Africa (SWA) during the summer monsoon months, and have an important cooling effect on the regional climate. Previous studies of these clouds have focused on modelling and remote sensing via satellite. We present the first comprehensive set of regional, in situ measurements of cloud microphysics, taken during June – July 2016, as part of the DACCIWA (Dynamics-Aerosol-Chemistry-Clouds Interactions in West Africa) campaign, assessing spatial and temporal variation in the properties of these clouds. LLC developed overnight and mean cloud cover peaked a few hundred kilometres inland around 10:00 local solar time (LST), before c…

Atmospheric Science010504 meteorology & atmospheric sciencesCloud coverPopulationclouds[SDU.STU.ME]Sciences of the Universe [physics]/Earth Sciences/Meteorology010502 geochemistry & geophysicsMonsoonAtmospheric sciences01 natural sciencescomplex mixtureslcsh:Chemistrylow level cloudsddc:550Cloud condensation nuclei1902WolkenphysikeducationSouthern Hemisphere0105 earth and related environmental sciencesOrographic lifteducation.field_of_studyaerosol effectmicropyhsicslcsh:QC1-999AerosolEarth scienceslcsh:QD1-99913. Climate action[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/ClimatologySolar timeEnvironmental sciencesense organs/dk/atira/pure/subjectarea/asjc/1900/1902lcsh:Physics
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In situ observations of new particle formation in the tropical upper troposphere: the role of clouds and the nucleation mechanism

2011

New particle formation (NPF), which generates nucleation mode aerosol, was observed in the tropical Upper Troposphere (UT) and Tropical Tropopause Layer (TTL) by in situ airborne measurements over South America (January–March 2005), Australia (November–December 2005), West Africa (August 2006) and Central America (2004–2007). Particularly intense NPF was found at the bottom of the TTL. Measurements with a set of condensation particle counters (CPCs) with different <i>d</i><sub>p50</sub> (50% lower size detection efficiency diameter or "cut-off diameter") were conducted on board the M-55 <i>Geophysica</i> in the altitude range of 12.0–20.5 km and on board …

Atmospheric Science010504 meteorology & atmospheric sciencesDISPERSION MODEL FLEXPARTaerosolnucleationNucleationclouds010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencestropicsTropospherelcsh:Chemistrynew particle formationddc:550Cloud condensation nucleiLife ScienceStratosphere0105 earth and related environmental sciencesGeophysica[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph][SDU.OCEAN]Sciences of the Universe [physics]/Ocean AtmosphereIce cloudAtmosphärische SpurenstoffeFalconlcsh:QC1-999AerosolJAQUEOUS SULFURIC-ACIDlcsh:QD1-99913. Climate actionClimatologyupper troposphereEnvironmental scienceOutflowAEROSOL NUCLEATIONLOWER STRATOSPHERETropopauselcsh:PhysicsGALACTIC COSMIC-RAYS
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Condensation nuclei at the German Antarctic Station “Georg von Neumayer”

1992

Evaluations of measurements of the tropospheric surface condensation nuclei at the German Antarctic station for the last 8 years are presented. They show clearly the annual variation of the concentration with a maximum in austral summer, as previously seen by other investigators. In addition, a pronounced increase of the concentration of 9.63% per year has been found. The size distributions of the condensation nuclei of measurements over 2 years are evaluated and discussed. On average, they are of mono-modal shape, but individually most of them show a bimodal shape. DOI: 10.1034/j.1600-0889.1992.00009.x

Atmospheric Science010504 meteorology & atmospheric sciencesMeteorology010501 environmental sciencesAtmospheric sciences01 natural scienceslanguage.human_languageTroposphereGermanlanguageCloud condensation nucleiEnvironmental scienceAnnual variation0105 earth and related environmental sciencesTellus B: Chemical and Physical Meteorology
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