Search results for "SMALL-SCALE ANISOTROPY"

showing 3 items of 3 documents

EUSO Science

2005

EUSO is a mission to explore the extreme universe by the probe of Ultra High Energy Cosmic Rays (LTHECRs) and LTHE neutrinos [1]. EUSO monitors a gigantic volume of atmosphere from Space and measures showers induced by UHECRs and UHE neutrinos. Scientifically, it is important to measure the energy spectrum of UHECRs well beyond GZK energy with high statistics. EUSO ensures the observation of UHECRs up to 10(21) eV even in the case of GZK mechanism working [2-7], and gives us a clear picture of the existence / non-existence of the GZK effect and the behavior of the spectrum beyond GZK energy, which represents the contributions from nearby sources. The anisotropy study of UHECR arrival direct…

ENERGY COSMIC-RAYSSPECTRUMSMALL-SCALE ANISOTROPY
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A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory

2012

Observations of cosmic ray arrival directions made with the Pierre Auger Observatory have previously provided evidence of anisotropy at the 99% CL using the correlation of ultra high energy cosmic rays (UHECRs) with objects drawn from the Véron-Cetty Véron catalog. In this paper we report on the use of three catalog independent methods to search for anisotropy. The 2pt–L, 2pt+ and 3pt methods, each giving a different measure of selfclustering in arrival directions, were tested on mock cosmic ray data sets to study the impacts of sample size and magnetic smearing on their results, accounting for both angular and energy resolutions. If the sources of UHECRs follow the same large scale structu…

HIRES STEREO[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomySMALL-SCALE ANISOTROPYAstrophysics01 natural sciencesAltas energíasCosmic Rays ShowerCosmologyUltra-high-energy cosmic rayAnisotropy010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]BL-LACERTAEAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryRadiación cósmicaFísica nuclearOBJECTSAstrophysics - High Energy Astrophysical Phenomenacosmic ray experiments; ultra high energy cosmic raysACTIVE GALACTIC NUCLEIActive galactic nucleusmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raysearch for anisotropyultra high energy cosmic raysCosmic Ray[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsCiencias ExactasPierre Auger ObservatorySPECTRUMAstronomyFísicaAstronomy and AstrophysicsASTROFÍSICAUniverseGalaxyExperimental High Energy Physicsanisotrpycosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyJournal of Cosmology and Astroparticle Physics
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Embryotoxicity studies of tri-n-butyltin(IV) complexes of 5-[(E)-2-(aryl)-1-diazenyl]-2-hydroxybenzoic acid and 2-[(E)-2-(3-formyl-4-hydroxyphenyl)-1…

2005

The toxicity studies of free 5-[(E)-2-(aryl)-1-diazenyll-2-hydroxybenzoic acid and 2-[(E)-2-(3-formyl-4-hydroxyphenyl)-1-diazenyllbenzoic acid and their tri-n-butyltin(IV) complexes were evaluated by using sea urchin early developmental stages as recommended model organisms for toxicity tests. The novel complexes, as the parent tri-n-butyltin(IV) chloride (TBTCl), caused mitosis block and induced high embryonic mortality in sea urchin. Copyright (c) 2005 John Wiley & Sons, Ltd.

chemistry.chemical_classificationSPECTRUMAzo compoundbiologyStereochemistryCarboxylic acidArylSMALL-SCALE ANISOTROPYGeneral ChemistryPhenolic acidbiology.organism_classificationParacentrotus lividusENERGY COSMIC-RAYSInorganic Chemistrychemistry.chemical_compoundchemistrybiology.animalSphaerechinus granularisSea urchinBenzoic acidApplied Organometallic Chemistry
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