Search results for "Observatory"

showing 10 items of 329 documents

Cosmological waveguides for gravitational waves

1997

We study the linearized equations describing the propagation of gravitational waves through dust. In the leading order of the WKB approximation, dust behaves as a non-dispersive, non-dissipative medium. Taking advantage of these features, we explore the possibility that a gravitational wave from a distant source gets trapped by the gravitational field of a long filament of galaxies of the kind seen in the large scale structure of the Universe. Such a waveguiding effect may lead to a huge magnification of the radiation from distant sources, thus lowering the sensitivity required for a successful detection of gravitational waves by detectors like VIRGO, LIGO and LISA.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGravitational-wave observatoryGravitational waveSpeed of gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitational accelerationGeneral Relativity and Quantum CosmologyLIGOGravitational energyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Gravitational fieldGravitational redshiftPhysical Review D
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Holographic in-situ measurements of the spatial droplet distribution in stratiform clouds

1998

Ground based in-situ measurements on the small-scale structure of low-level stratiform clouds have been performed utilizing the HOlographic Droplet and Aerosol Recording system (HODAR) of the University of Mainz, Germany. 6 holograms recorded during stratus cloud events on the Kleiner Feldberg Taunus Mountain Observatory (Frankfurt, Germany) were reconstructed in the laboratory and analysed by means of an automated data extraction and image processing system. In post-processing, each originally recorded droplet population was subjected to 2 statistical methods: (1) the sub-cell scanning analyses with statistical “Fishing” tests and (2) measurements of inter-droplet distance frequency distri…

In situAtmospheric Scienceeducation.field_of_study010504 meteorology & atmospheric sciencesMeteorologyPopulationHolographyImage processing010501 environmental sciences01 natural sciencesAerosollaw.inventionDistribution (mathematics)ObservatorylawFrequency distributioneducationGeology0105 earth and related environmental sciencesRemote sensingTellus B: Chemical and Physical Meteorology
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La experiencia docente del Observatorio de derechos humanos en la formación de juristas comprometidos

2021

[EN] The Human Rights Observatory is a pilot experience based on the teaching-learning methodology that allows, in an open, dynamic and participatory way. It monitors international current affairs and opens up a space for discussion and debate in the classroom on all those phenomena that, to a greater or lesser extent, condition International Law in the contemporary world. For this purpose, the Observatory will raise questions about issues of interest, highly topical subjects, complex problems, controversial processes and, above all, new approaches that encourage, not only through autonomous work but also through critical reflection, to deepen and complement the theoretical content of the d…

Innovación educativaInnovaciónEducación superiorHuman rightsDerechos humanosEnseñanza superiorTecnologías y educaciónObservatoryInnovationReflexión críticaCritical thinkingObservatorio
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The THESEUS space mission concept: science case, design and expected performances

2018

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing …

IonizationAtmospheric Sciencecosmological modelCherenkov Telescope Array[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyDark ageMASSIVE SINGLE STARSStar formation rates Gamma ray01 natural sciencesCosmology: observationlocalizationlaw.inventionAstrophysicEinstein Telescopeobservational cosmologylawObservational cosmologyRe-ionizationCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionizationLIGOobservations [Cosmology]Telescope010303 astronomy & astrophysicsHigh sensitivityHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMulti-wavelengthenergy: highsezelegamma-ray burstsCosmology: observationsCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionization; Aerospace Engineering; Space and Planetary ScienceAstrophysics::Instrumentation and Methods for Astrophysicsimagingstar: formationburst [Gamma-ray]observatoryGeophysicsDark agesX rays Cosmology: observationAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenasignatureStarTIDAL DISRUPTIONGamma-ray: burstAstrophysics::High Energy Astrophysical PhenomenaSIMILAR-TO 6Socio-culturaleFOS: Physical sciencesAerospace EngineeringGamma-ray: burstsobservation [Cosmology]galaxy: luminosityX-ray astronomy: instrumentation7 CANDIDATE GALAXIESAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burst114 Physical sciencesSettore FIS/03 - Fisica della MateriaTelescopeX-raybursts [Gamma-ray]FIS/05 - ASTRONOMIA E ASTROFISICASettore FIS/05 - Astronomia e AstrofisicaFirst star0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]KAGRAInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsFirst starsLIGHT CURVESEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and Astrophysics115 Astronomy Space scienceCherenkov Telescope ArrayredshiftsensitivityRedshiftNEUTRON-STAR MERGERmessengerVIRGOelectromagneticLUMINOSITY FUNCTIONSpace and Planetary ScienceBLACK-HOLEGeneral Earth and Planetary SciencesGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Cosmic ray composition and energy spectrum from 1–30 PeV using the 40-string configuration of IceTop and IceCube

2012

Astroparticle physics 42, 15 - 32 (2013). doi:10.1016/j.astropartphys.2012.11.003

Knee regionAstrophysicsTracking (particle physics)01 natural sciencesParticle identificationIceCubeTRACKINGWATERCherenkovNeutrino energyNEUTRINO TELESCOPEUltra-high-energy cosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSEADetectorAstrophysics::Instrumentation and Methods for AstrophysicsLIGHTComposition; Cosmic rays; Energy spectrum; IceCube; IceTop; Knee regionddc:540IceTopPARTICLE IDENTIFICATIONAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsIceCube detectorCompositionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2IceCube Neutrino ObservatorySEARCHESAccelerationcosmic raysdE/dx0103 physical sciences010306 general physicsDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)Cherenkov radiationTruncated meanMuon energy010308 nuclear & particles physicsAstronomyAstronomy and Astrophysics540Physics and AstronomycompositionEnergy SpectrumTEVEnergy spectrum
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Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory

2011

We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 × 1017 eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.

Large scale anisotripies[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Auger ExperimentAstronomyAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)FOS: Physical sciencesCosmic rayAstrophysicsanisotropySURFACE DETECTOR01 natural sciencesCosmic RayAugerLarge scale anisotropiesObservatoryLarge scale anisotropie0103 physical sciences010303 astronomy & astrophysicsUltra-high energy cosmic rayCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryFÍSICA DE PARTÍCULASUltra High Energy Cosmic Rays.010308 nuclear & particles physicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsPierre Auger ObservatoryUltra-high energy cosmic raysENERGY-SPECTRUMRadiación cósmicaAnisotropíaAmplitudeHarmonicsUltra-high energy cosmic rays; Large scale anisotropies; Pierre Auger ObservatoryExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearRight ascensionAstrophysics - High Energy Astrophysical Phenomena
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Astronomiskajam tornim - 150

2019

Latvijas Universitātes Muzeja virtuālā izstāde „Astronomiskajam tornim – 150” veltīta labi pamanāmai Latvijas Universitātes galvenās ēkas iezīmei – Astronomiskajam tornim uz tās jumta. 2019. gadā ēkai un arī tornim apritēja 150 gadi. Rīgas Politehnikuma laikos te strādājuši dažādi ārzemju profesori, kas veica astronomiskus novērojumus un mācīja studentus. Nodibinoties Latvijas Universitātei, tornis kļuva par Astronomiskās observatorijas sastāvdaļu. Kopš 1986. gada te notiek regulāri debess spīdekļu demonstrējumi, skatītas komētas, Saules aptumsumi un citas samērā retas astronomiskas parādības. Astronomiskais tornis ir kā logs uz debesīm vairāk nekā 150 gadu garumā. Mainījušies teleskopi, no…

Latvijas Universitāte:NATURAL SCIENCES::Physics::Astronomy and astrophysics::Astronomy [Research Subject Categories]telescopesRaiņa bulvāris 19University of LatviateleskopiastronomyAstronomical ObservatoryRiga PolytechnicAstronomiskā observatorijaastronomijaAstronomiskais tornisRīgas PolitehnikumsAstronomical tower
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Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

2014

Made available in DSpace on 2022-04-29T07:21:49Z (GMT). No. of bitstreams: 0 Previous issue date: 2014-11-17 We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of …

MECHANISMPhysics and Astronomy (miscellaneous)AstrophysicsFOLLOW-UP OBSERVATIONSASTROPHYSICAL SOURCESIceCubeneutrinoDetection of gravitational waveGravitational waves neutrinoObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCLIGO Scientific CollaborationQBPhysicsGAMMA-RAY BURSTS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYNuclear and High Energy Physics; Physics and Astronomy (miscellaneous)NEUTRINOSNeutrino detectorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGNeutrinoSENSITIVITYGIANT FLARENuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]95.85.RyMUON NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATIONGravitational wavesGeneral Relativity and Quantum CosmologyINSTABILITIESSettore FIS/05 - Astronomia e AstrofisicaCORE-COLLAPSE SUPERNOVAE[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530SDG 7 - Affordable and Clean EnergyCORE-COLLAPSEDETECTOR/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyGravitational wave95.85.SzMAGNETIZED NEUTRON-STARS[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyTRANSIENTS95.85.Sz; 95.85.RyRELATIVISTIC STARSLIGOPhysics and Astronomy[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Gamma-ray burstEMISSIONEnergy (signal processing)
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Conceptual design of the International Axion Observatory (IAXO)

2014

The International Axion Observatory (IAXO) will be a forth generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar plasma photons. In terms of signal-to-noise ratio, IAXO will be about 4-5 orders of magnitude more sensitive than CAST, currently the most powerful axion helioscope, reaching sensitivity to axion-photon couplings down to a few $\times 10^{-12}$ GeV$^{-1}$ and thus probing a large fraction of the currently unexplored axion and ALP parameter space. IAXO will also be sensitive to solar axions produced by mechanisms mediated by the axion-electron coupling $g_{…

MICROPICPhysics - Instrumentation and DetectorsPhotonaxionsParameter space7. Clean energyHigh Energy Physics - ExperimentDark Matter detectors (WIMPs axions etc.)High Energy Physics - Experiment (hep-ex)Observatoryetc.)Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc)Detectors and Experimental TechniquesInstrumentationMathematical PhysicsPhysicsGEMsolar [axion]Dark Matter Detectors (Wimps Axions etc.)MicroMegas detectorX-ray detectorsInstrumentation and Detectors (physics.ins-det)Dark Matter detectors (WIMPs axions etc.); Large detector systems for particle and astroparticle physics; Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc); X-ray detectors; Instrumentation; Mathematical PhysicssolarobservatoryMICROMEGASMHSPaxion-like particlesproposed experimentaxions ; dark matter detectors ; x-ray detectors ; Micropattern gaseous detectors ; large detector systems for particle and astroparticle physicsMicromegasX-ray detectorParticle physicsoptics [X-ray]FOS: Physical sciencesSuperconducting magnetMicropattern gaseous detectors (MSGCddc:610Axionactivity reportDark Matter detectors (WIMPssuperconductivity [magnet]etc)HelioscopeLarge detector systems for particle and astroparticle physicssensitivityInGridRETHGEMOrders of magnitude (time)axionLarge detector systems for particle and astroparticle physicTHGEMMicropattern Gaseous Detectors (MSGC Gem THGEM Rethgem MHSP Micropic Micromegas In Grid; etc)
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Simulating AIA observations of a flux rope ejection

2014

D.H.M. would like to thank STFC, the Leverhulme Trust and the European Commission’s Seventh Framework Programme (FP7/2007-2013) for their financial support. P.P. would like to thank the European Commission’s Seventh Framework Programme (FP7/2007-2013) under grant agreement SWIFF (project 263340, http://www.swiff.eu) and STFC for financial support. These results were obtained in the framework of the projects GOA/2009-009 (KU Leuven), G.0729.11 (FWO-Vlaanderen) and C 90347 (ESA Prodex 9). The research leading to these results has also received funding from the European Commission’s Seventh Framework Programme (FP7/2007-2013) under the grant agreements SOLSPANET (project No. 269299, http:// ww…

Magnetohydrodynamics (MHD)corona [Sun]Sun: coronal mass ejections (CMEs)FOS: Physical sciencesAstrophysicsmagnetohydrodynamics (MHD)7. Clean energyProminencesObservatoryRadiative transferQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsQASun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)QBPhysicsUV radiation [Sun]Line-of-sightSun: coronaAstronomy and AstrophysicsPlasmaSun: UV radiationCoronacoronal mass ejections (CMEs) [Sun]Magnetic fluxSun: filamentsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]13. Climate actionSpace and Planetary ScienceExtreme ultravioletPhysics::Space Physicsfilaments prominences [Sun]Rope
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