Search results for "programming."

showing 10 items of 3035 documents

IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae ( Corrigendum )

2014

Keywords: neutrinos ; supernovae: general ; instrumentation: detectors ; errata ; addenda Reference EPFL-ARTICLE-198916doi:10.1051/0004-6361/201117810eView record in Web of Science Record created on 2014-05-19, modified on 2017-05-12

PhysicsSupernovaLow energyWeb of scienceSpace and Planetary Scienceddc:520Astronomy and AstrophysicsAstrophysicsInstrumentation (computer programming)Sensitivity (control systems)Neutrino
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Reduction of the uncertainty in the measurements of magnetic fields

2014

The paper deals with magnetic field measurement, carried out by using a broadband and isotropic instrument. These measurements are characterized by a very high uncertainty values if compared with the ones usually related to other electrical measurements. For these reasons, if the measurements are performed to assess the exposure of human beings, these large uncertainty values imply a high risk of wrong decision when there is the need to establish if a site complies or does not comply with a specified emission limits. A reduction of the uncertainty values implies a reduction of the risk. With this aim, we propose an approach which, in particular but very typical cases, allows an effective re…

PhysicsSustainability and the EnvironmentMagnetoresistancebusiness.industrymagnetic field measurementsIsotropyElectrical engineeringmeasurement uncertainty.Magnetic fieldReduction (complexity)Control theorymagnetic field measurementmeasurement uncertaintyCalibrationSettore ING-IND/09 - Sistemi per l'Energia e L'AmbienteMeasurement uncertaintyElectrical measurementsRenewable EnergyInstrumentation (computer programming)businessSettore ING-INF/07 - Misure Elettriche E Elettronichemagnetic field measurements; measurement uncertainty; Renewable Energy Sustainability and the Environment2014 International Conference on Renewable Energy Research and Application (ICRERA)
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Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine

2007

We present a detailed analysis of Swift multi-wavelength observations of GRB 070110 and its remarkable afterglow. The early X-ray light curve, interpreted as the tail of the prompt emission, displays a spectral evolution already seen in other gamma-ray bursts. The optical afterglow shows a shallow decay up to ~2 d after the burst, which is not consistent with standard afterglow models. The most intriguing feature is a very steep decay in the X-ray flux at ~20 ks after the burst, ending an apparent plateau. The abrupt drop of the X-ray light curve rules out an external shock as the origin of the plateau in this burst and implies long-lasting activity of the central engine. The temporal and s…

PhysicsSwiftAstrophysics::High Energy Astrophysical PhenomenaSpectral propertiesAstrophysics (astro-ph)X-rayPhase pointFOS: Physical sciencesGamma Rays: Bursts; X-rays: individual (GRB 070110)Astronomy and AstrophysicsAstrophysicsAstrophysicsLight curveAfterglowGamma Rays: BurstsSpace and Planetary ScienceMillisecond pulsarGamma-ray burstcomputerX-rays: individual (GRB 070110)computer.programming_language
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Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era

2015

Between 2011 March and 2014 August Swift responded to 20 triggers from the IceCube neutrino observatory, observing the IceCube 50% confidence error circle in X-rays, typically within 5 hours of the trigger. No confirmed counterpart has been detected. We describe the Swift follow up strategy and data analysis and present the results of the campaign. We discuss the challenges of distinguishing the X-ray counterpart to a neutrino trigger from serendipitous uncatalogued X-ray sources in the error circle, and consider the implications of our results for future strategies for multi-messenger astronomy, with particular reference to the follow up of gravitational wave triggers from the advanced-era…

PhysicsSwiftHigh Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaAstronomyLibrary scienceFOS: Physical sciencesAstronomy and AstrophysicsMethods observationalLIGOSpace and Planetary Scienceddc:520Astrophysics - High Energy Astrophysical Phenomenacomputercomputer.programming_language
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The Status of the Ultra Fast Flash Observatory - Pathfinder

2012

On behalf of the UFFO Collaboration; International audience; The Ultra Fast Flash Observatory (UFFO) is a project to study early optical emissions from Gamma Ray Bursts (GRBs). The primary scientific goal of UFFO is to see if GRBs can be calibrated with their rising times, so that they could be used as new standard candles. In order to minimize delay in optical follow-up measurements, which is now about 100 sec after trigger from the Swift experiment, we rotate a mirror to redirect light path so that optical measurement can be performed within a second after the trigger. We have developed a pathfinder mission, UFFO-pathfinder to launch on board the Lomonosov satellite in 2012. In this talk,…

PhysicsSwiftNuclear and High Energy Physics[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]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyCosmic ray01 natural sciencesAtomic and Molecular Physics and OpticsEarly Light Emissions[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Flash (photography)PathfinderObservatory0103 physical sciencesGamma Ray BurstsUltra fastSatelliteGamma-ray burst010303 astronomy & astrophysicscomputerUltra Fast Flash Observatorycomputer.programming_language
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Grid-based Methods in Relativistic Hydrodynamics and Magnetohydrodynamics

2015

An overview of grid-based numerical methods used in relativistic hydrodynamics (RHD) and magnetohydrodynamics (RMHD) is presented. Special emphasis is put on a comprehensive review of the application of high-resolution shock-capturing methods. Results of a set of demanding test bench simulations obtained with different numerical methods are compared in an attempt to assess the present capabilities and limits of the various numerical strategies. Applications to three astrophysical phenomena are briefly discussed to motivate the need for and to demonstrate the success of RHD and RMHD simulations in their understanding. The review further provides FORTRAN programs to compute the exact solution…

PhysicsTest benchRelativistic hydrodynamics (RHD)FortranNumerical analysisReview ArticleGridlaw.inventionsymbols.namesakeRiemann problemExact solutions in general relativitylawPhysics::Space PhysicssymbolsCartesian coordinate systemStatistical physicsMagnetohydrodynamicscomputerRelativistic magnetohydrodynamics (RMHD)computer.programming_languageLiving Reviews in Computational Astrophysics
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Stable control of pulse speed in parametric three-wave solitons.

2006

International audience; We analyze the control of the propagation speed of three wave packets interacting in a medium with quadratic nonlinearity and dispersion. We find analytical expressions for mutually trapped pulses with a common velocity in the form of a three-parameter family of solutions of the three-wave resonant interaction. The stability of these novel parametric solitons is simply related to the value of their common group velocity.

Physics[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Analytical expressionsWave packetMathematical analysisDispersion (waves); parameter estimation; quadratic programmingFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesStability (probability)Physics - Plasma Physics010305 fluids & plasmasPulse (physics)Plasma Physics (physics.plasm-ph)Classical mechanics[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Dispersion relation0103 physical sciencesDispersion (optics)Group velocity010306 general physicsOptics (physics.optics)Parametric statisticsPhysics - OpticsPhysical review letters
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Geometric Origin of the Tennis Racket Effect

2020

The tennis racket effect is a geometric phenomenon which occurs in a free rotation of a three-dimensional rigid body. In a complex phase space, we show that this effect originates from a pole of a Riemann surface and can be viewed as a result of the Picard-Lefschetz formula. We prove that a perfect twist of the racket is achieved in the limit of an ideal asymmetric object. We give upper and lower bounds to the twist defect for any rigid body, which reveals the robustness of the effect. A similar approach describes the Dzhanibekov effect in which a wing nut, spinning around its central axis, suddenly makes a half-turn flip around a perpendicular axis and the Monster flip, an almost impossibl…

Physics[PHYS]Physics [physics]Riemann surfaceGeneral Physics and AstronomyClassical Physics (physics.class-ph)FOS: Physical sciencesMathematical Physics (math-ph)Physics - Classical PhysicsRigid body01 natural sciencesUpper and lower boundssymbols.namesakePerpendicular AxisClassical mechanics[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]Phase space0103 physical sciencesRacketsymbolsIdeal (ring theory)Twist010306 general physicscomputerMathematical Physicscomputer.programming_language
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An Astronomical Observatory in the Classroom

2005

We describe a project developed at the University of Granada in collaboration with the Instituto de Astrofisica de Andalucia aimed at using a remote telescope for live astronomical observations from the classroom. Available instrumentation, software and activities are presented.

Physicsbusiness.industryGeneral EngineeringAstronomy and AstrophysicsAstrophysicslaw.inventionTelescopeSoftwareSpace and Planetary ScienceObservatorylawSystems engineeringInstrumentation (computer programming)businessEAS Publications Series
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Legri Science Operation Center. Architecture and Operations

2001

The LEGRI Science Operation Center (SOC) is the single contact point between the MINISAT-01 Centro de Operaciones Cientificas (COC) located at Villafranca del Castillo (Madrid) and the LEGRI Consortium. Its architecture, operational procedures and associated software has been developed at the Universities of Valencia and Birmingham on the scope to define a integrated Data Analysis System, able to perform the daily follow-up of the instrument health, raw data files decompression and archiving activities (on-line and historical). Pointing and telecommand files generation are also SOC responsibilities. The aim of this paper is to report the SOC activities during the two years of LEGRI operatio…

Physicsbusiness.industrycomputer.software_genreData processing systemTelecommandAlpha (programming language)SoftwareOperating systemInstrumentation (computer programming)ArchitectureRaw databusinesscomputerScope (computer science)
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