Search results for "Pie"

showing 10 items of 4404 documents

A search for point sources of EeV neutrons

2012

A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from −90◦ to +15◦ in declination using four different energy ranges above 1 EeV (1018 eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions for each of the four energy ranges. These results constrain scenarios for the production of ultrahigh energy cosmic rays in the Galaxy.

AstronomyEnergy fluxAstrophysics01 natural sciences7. Clean energyNeutron fluxObservatorycosmic rays – Galaxy: disk – methods: data analysisNeutron detection010303 astronomy & astrophysicsHigh 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]Gamma rayAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYPierre Auger ObservatoryCOSMIC-RAYSRadiación cósmicaUltra High Energy Cosmic RayComputingMethodologies_DOCUMENTANDTEXTPROCESSINGMASSIVE BLACK-HOLEFísica nuclearPierre Auger Observatory high-energy neutron sources neutron flux limitAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayGalaxiaGalaxy: diskcosmic rays0103 physical scienceshigh-energy neutron sourcesNeutronCosmic-ray observatoryCiencias ExactasANISOTROPY010308 nuclear & particles physicsGAMMA-RAYSAnálisis de datosAstronomyFísicaAstronomy and AstrophysicsASTROFÍSICAneutron flux limitmethods: data analysisNÊUTRONSSpace and Planetary ScienceUltra High Energy Cosmic RaysExperimental High Energy Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]GALACTIC-CENTER
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The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory

2021

FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stellar photometry. As a passive system which does not produce any light that could interfere with the observations of the fluorescence telescopes of the observatory, it complements the active monitoring systems that use lasers. We discuss the applications of stellar photometry for atmospheric monitoring at optical observatories in general and the particular modes of operation employed by the Auger FRAM. We describe in detail the technical aspects of FRAM, the hardware and software requirements for a successful operati…

AstronomyLarge detector systems for particle and astroparticle physics; Optics; Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Real-time monitoringReal-time monitoring01 natural sciencesAugerSuccessful operationObservatoryopticalAPDshardwareAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsInstrumentationPhoton detectors for UVMathematical PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEEBCCDsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSi-PMTsAugerobservatoryRobotic telescopeG-APDsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSciences exactes et naturellesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesprogrammingdetector: fluorescencePhotometry (optics)0103 physical sciencesddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]High Energy Physicsvisible and IR photons (solid-state) (PIN diodesCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsRemote sensingetc)fluorescence [detector]Pierre Auger Observatory010308 nuclear & particles physicsLarge detector systems for particle and astroparticle physicsActive monitoringOpticsCCDslasermonitoringEMCCDsLarge detector systems for particle and astroparticle physicatmosphereExperimental High Energy PhysicsOpticEnvironmental science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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An Indication of Anisotropy in Arrival Directions of Ultra-high-energy Cosmic Rays through Comparison to the Flux Pattern of Extragalactic Gamma-Ray …

2018

A new analysis of the dataset from the Pierre Auger Observatory provides evidence for anisotropy in the arrival directions of ultra-high-energy cosmic rays on an intermediate angular scale, which is indicative of excess arrivals from strong, nearby sources. The data consist of 5514 events above 20 EeV with zenith angles up to 80 deg recorded before 2017 April 30. Sky models have been created for two distinct populations of extragalactic gamma-ray emitters: active galactic nuclei from the second catalog of hard Fermi-LAT sources (2FHL) and starburst galaxies from a sample that was examined with Fermi-LAT. Flux-limited samples, which include all types of galaxies from the Swift-BAT and 2MASS …

Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Ciencias Físicascosmic radiation: densitygalaxies: starburstAstrophysics01 natural sciences//purl.org/becyt/ford/1 [https]methods: data analysis Supporting material: FITS fileUltra-high-energy cosmic raydata analysis [Methods]Anisotropycosmic radiation: model010303 astronomy & astrophysicscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOBSERVATÓRIOSSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files; Astronomy and Astrophysics; Space and Planetary ScienceAugerobservatorygamma ray: emissiondata analysis Supporting material: FITS file [methods]astroparticle physicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusactive [Galaxies]Astrophysics::High Energy Astrophysical Phenomenagalaxies: activeData analysisFOS: Physical sciencesStarburstCosmic rayanisotropyAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias FísicasGLASTcosmic raysastroparticle physics; cosmic rays; galaxies: active; galaxies: starburst; methods: data analysis Supporting material: FITS files0103 physical sciencesHigh Energy Physicscosmic radiation: UHEAGNCosmic raysAstrophysics::Galaxy AstrophysicsZenithmethods: data analysis Supporting material: FITS filesPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsIsotropyFísicaAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]Astronomy and Astrophysicmethods: data analysisGalaxyfluxstarburst [Galaxies]Space and Planetary ScienceExperimental High Energy PhysicsActive galaxiesgalaxyAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]statistical
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Large-scale Cosmic-Ray Anisotropies above 4 EeV Measured by the Pierre Auger Observatory

2018

We present a detailed study of the large-scale anisotropies of cosmic rays with energies above 4 EeV measured using the Pierre Auger Observatory. For the energy bins [4,8] EeV and $E\geq 8$ EeV, the most significant signal is a dipolar modulation in right ascension at energies above 8 EeV, as previously reported. In this paper we further scrutinize the highest-energy bin by splitting it into three energy ranges. We find that the amplitude of the dipole increases with energy above 4 EeV. The growth can be fitted with a power law with index $\beta=0.79\pm 0.19$. The directions of the dipoles are consistent with an extragalactic origin of these anisotropies at all the energies considered. Addi…

Astronomymagnetic fieldAstrophysicsAstrophysics01 natural sciencesAmplitudeastroparticle physics; cosmic raysAnisotropy010303 astronomy & astrophysicscosmic rayastroparticle physics cosmic raysRight ascensionHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HECOSMIC cancer databaseORIGINOBSERVATÓRIOSPhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicAugerastroparticle physics; cosmic rays; Astronomy and Astrophysics; Space and Planetary ScienceobservatorymodulationAmplitudeastroparticle physicsCosmic cancer databaseAstrophysics - High Energy Astrophysical Phenomenalarge scale anysotropysplittingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayContext (language use)cosmic radiation: anisotropycosmic rays0103 physical sciencesHigh Energy Physicscosmic radiation: UHEPierre auger observatoryPierre Auger Observatoryextragalactic origin010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsContext (language use)Astronomy and AstrophysicCosmic rayDipoleSpace and Planetary ScienceExperimental High Energy PhysicsAnisotropyDipoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Right ascensionlarge scale anysotropy extragalactic origindipole
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Erratum to "Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory"[Astroparticle Physics 32…

2010

The Pierre Auger Collaboration... K.B. Barber... J.A. Bellido... R.W. Clay... B.R. Dawson... V.C. Holmes... J. Sorokin... P. Wahrlich... B.J. Whelan... M.G. Winnick... et al.

Astroparticle physicsPhysicsPierre Auger Observatory[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010308 nuclear & particles physicsAstronomyDetectorAstronomyAstronomy and AstrophysicsAstrophysics01 natural sciencesAuger[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Experimental High Energy Physics0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstroparticle Physics
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Starpzvaigžņu putekļu virsmas un mantijas ķīmisko procesu makroskopiskā Montekarlo modelēšana

2018

No starpzvaigžņu vides novērojumiem konstatēts, ka ap starpzvaigžņu putekļa kodolu aukstos apstākļos (T~10 K) aug ledus apvalciņš no apkārtējās vides gāzes vielām, kuras piesalst pie šī putekļa. Ledus apvalciņu var ķīmiski diferencēt virsmā un mantijā. Šī ledus apvalka virsma un mantija ļauj veidoties sarežģītām molekulām starpzvaigžņu vidē. Tagad nāk daudz spektroskopisku datu par to kā šie putekļi palīdz veidoties sarežģītām un pat organiskām molekulām, ir nepieciešams izveidot modeļus, kas saskaņā ar šiem datiem spēs modelēt starpzvaigžņu vides reakciju kinētiku un palīdzēs izskaidrot kompleksu molekulu rašanos starpzvaigžņu vidē. Ņemot vērā to, ka puteklis sastāv no maza skaita molekulu…

Astroķīmijastarpzvaigžņu putekļiFizikaDžilespie algoritmsreakciju kinētika
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Immersīva pieeja kā mācību metode attālinātajās mācībās teātra mākslā 1.-3. klasē

2021

Ksenias Drovnikovas pieredzes darbs otrā līmeņa profesionālās augstākās izglītības programmā “Skolotājs” Immersīva pieeja kā mācību metode attālinātajās mācībās teātra mākslā 1.-3. klasē izstrādāts vadībā Mag. Paed. Ligitas Smildziņas 2021. gadā. Pieredzes darba mērķis ir īstenot attālināto mācību nodarbības teātra mākslā 1.-3. klašu vecumposmam, izmantojot immersīva teātra metodiku. Pieredzes darba uzdevumi ir izpētīt attālināto mācību procesa īpatnības un immersīva teātra metodiku, kā līdzekli attālināto mācību programmas īstenošanai, noteikt mācību metodes teātra mākslā attālinātām mācībām, praktiski realizēt immersīva teātra metodiku attālinātās mācībās. Tiek izmantotas teorētiskās meto…

Atbildīgs pieaugušaisIzglītības zinātnesImmersīva pieejaAttālinātās mācībasTeātra mākslaVērtēšana
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Vispārzināma fakta jēdziens civilprocesā

2022

Bakalaura darba tēma ir “Vispārzināma fakta jēdziens civilprocesā”. Darba mērķis ir noskaidrot, pēc kādiem kritērijiem vērtējams vai fakts ir uzskatāms par vispārzināmu un, līdz ar to, no kādu faktu pierādīšanas atbrīvojami lietas dalībnieki, kā arī analizēt, kā šis jautājums tiek risināts Latvijas tiesu praksē. Lai sasniegtu šī darba mērķi, autors ir aplūkojis dažādas publikācijas, interneta resursus un normatīvos aktus gan latviešu, gan angļu valodā, kā arī analizējis Latvijas Republikas tiesu praksi.

Atbrīvošana no pierādīšanasVispārzināms faktsPierādīšanas pienākumsPierādīšanaJuridiskā zinātne
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Formatīvās vērtēšanas paņēmieni ķīmijā pamatskolā

2016

Formatīvās vērtēšanas paņēmieni ķīmijā pamatskolā. Darba autore Tālberga M., darba vadītāja Mg. ķīm. Gaile I. Bakalaura darbs, 44 lappuses, 26 attēli, 3 tabulas, 23 literatūras avoti, 14 pielikumi. Latviešu valodā. Darba mērķis ir izpētīt formatīvās vērtēšanas pieejas, lai uzlabotu skolēnu mācīšanās procesu. Darbā ir literatūras un avotu apskats par vērtēšanu, formatīvo vērtēšanu un formatīvās vērtēšanas pieeju izvēli pamatskolā. Darba pētnieciskajā daļā izstrādātas un aprobētas mācību stundas tematā „Gaiss un tā kvalitāte’’. Veikta stundu analīze. Izstrādāts un aprobēts noslēguma darbs. Veikta skolēnu anketēšana, lai noskaidrotu viedokli par mācību procesu ķīmijas priekšmetā, tematā „Gaiss…

Atgriezeniskā saitePedagoģijaFormatīvā vērtēšanaFormatīvās vērtēšanas pieejasVērtēšana
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Origin of atmospheric aerosols at the Pierre Auger Observatory using studies of air mass trajectories in South America

2014

The Pierre Auger Observatory is making significant contributions towards understanding the nature and origin of ultra-high energy cosmic rays. One of its main challenges is the monitoring of the atmosphere, both in terms of its state variables and its optical properties. The aim of this work is to analyze aerosol optical depth $\tau_{\rm a}(z)$ values measured from 2004 to 2012 at the observatory, which is located in a remote and relatively unstudied area of the Pampa Amarilla, Argentina. The aerosol optical depth is in average quite low - annual mean $\tau_{\rm a}(3.5~{\rm km})\sim 0.04$ - and shows a seasonal trend with a winter minimum - $\tau_{\rm a}(3.5~{\rm km})\sim 0.03$ -, and a sum…

Atmospheric Science010504 meteorology & atmospheric sciencesaerosolAstronomyObservatoriesAerosol concentrationAir pollution010501 environmental sciencesAtmospheric sciencesmedicine.disease_causeAerosols Atmospheric aerosols Augers Cosmic rays Observatories; Aerosol concentration Aerosol optical depths Air mass Atmospheric effects GDAS HYSPLIT Pierre Auger observatory Ultra high-energy cosmic rays; Meteorology; aerosol property air mass concentration (composition) optical depth trajectory urban area urban atmosphere; Argentina01 natural sciencesoptical depthObservatory11. Sustainabilityddc:550MeteorologiaAugersmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsconcentration (composition)Physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]urban atmosphereAtmospheric effectsGDASAtmospheric aerosolscosmic ray; aerosol; air masses; atmospheric effectPhysics - Atmospheric and Oceanic PhysicstrajectoryClimatologyComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHYSPLITAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaPollutionaerosol property[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]media_common.quotation_subjectatmospheric effectArgentinaFOS: Physical sciencesHYSPLITAtmósferaAtmosphereMeteorologycosmic raysmedicineAerosol optical depthsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysCiencias ExactasAir mass0105 earth and related environmental sciencesAerosols[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Pierre Auger ObservatoryFísicaASTROFÍSICA[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Aerosol13. Climate actionExperimental High Energy PhysicsAtmospheric and Oceanic Physics (physics.ao-ph)Pierre Auger observatoryAir massair massesUltra high-energy cosmic raysurban area
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