Objektiviertes Beurteilungsverfahren für Sichtbeton mittels automatisierter Bildverarbeitung unter Berücksichtigung von Beleuchtungsvariationen

Es wird ein Verfahren vorgestellt, das erlaubt, die Vermessung von Porengrößen in Sichtbetonflächen sowie die Beurteilung von Farbeindrücken automatisiert durchzuführen. Subjektive Einflüsse bei der Bewertung werden ausgeschlossen, gleichzeitig werden Einsparungseffekte von 80% und mehr gegenüber Handauszählungen von Lunkern nachgewiesen. Die verwendeten Techniken sind ein spezieller Markierungsrahmen, eine hochauflösende Digitalkamera und spezielle Bildanalyseprozeduren. Letztere leisten die notwendigen Vorverarbeitungsfunktionen, wie geometrische Entzerrung, Kalibrierung sowie einen Helligkeitsausgleich, und nehmen die durchzuführenden Bewertungen vor. Das sind Porengrößen- und verteilungsanalyse sowie Farbvergleiche mit definierten Normalen zur Beurteilung von Farbhomogenitäten über den zu analysierenden Sichtbetonflächen. Die Ergebnisprotokollierung erfolgt sowohl bildlich als auch datentechnisch, letzteres z. B. in einem Excelfile. Die Durchgängigkeit des Verfahrens wird an einer Reihe von in Sichtbetonbauweise ausgeführten Bauten veranschaulicht, z. B. dem Bundeskanzleramt und dem Hörsaalzentrum der TU-Dresden. Wesentliche Einflussparameter wie Beleuchtungsgeometrie oder Helligkeitsschwellen werden diskutiert und Vergleiche zu durchgeführten Handmessungen gezogen. Der vorgestellte Ansatz ist in weiterer Forschung anwendungsorientiert aufzubereiten, vergleichende Untersuchungen zu durch Experten durchgeführten Messungen sind zu Validierungszwecken vorzunehmen. Der Ansatz kann einen Beitrag zu Normungsfragen liefern. Seine Nutzbarkeit ist auch für spezielle Bereiche der Entwicklung von Betonmischtechnologien oder in der Fertigelementefertigung gegeben. Im Beitrag sind die relevanten Verfahrensschritte bildlich und in tabellarischer Form untersetzt

Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO 600, LIGO, and Virgo detectors

Paper producido por "The LIGO Scientific Collaboration and the Virgo Collaboration". (En el registro se mencionan solo algunos autores de las decenas de personas que participan).In this paper we report on a search for short-duration gravitational wave bursts in the frequency range 64 Hz–1792 Hz associated with gamma-ray bursts (GRBs), using data from GEO 600 and one of the LIGO or Virgo detectors. We introduce the method of a linear search grid to analyze GRB events with large sky localization uncertainties, for example the localizations provided by the Fermi Gamma-ray Burst Monitor (GBM). Coherent searches for gravitational waves (GWs) can be computationally intensive when the GRB sky position is not well localized, due to the corrections required for the difference in arrival time between detectors. Using a linear search grid we are able to reduce the computational cost of the analysis by a factor of Oð10Þfor GBM events. Furthermore, we demonstrate that our analysis pipeline can improve upon the sky localization of GRBs detected by the GBM, if a high-frequency GW signal is observed in coincidence. We use the method of the linear grid in a search for GWs associated with 129 GRBs observed satellite-based gamma-ray experiments between 2006 and 2011. The GRBs in our sample had not been previously analyzed for GW counterparts. A fraction of our GRB events are analyzed using data from GEO 600 while the detector was using squeezed-light states to improve its sensitivity; this is the first search for GWs using data from a squeezed-light interferometric observatory. We find no evidence for GW signals, either with any individual GRB in this sample or with the population as a whole. For each GRB we place lower bounds on the distance to the progenitor, under an assumption of a fixed GWemission energy of 10−2M⊙c2, with a median exclusion distance of 0.8 Mpc for emission at 500 Hz and 0.3 Mpc at 1 kHz. The reduced computational cost associated with a linear search grid will enable rapid searches for GWs associated with Fermi GBM events once the advanced LIGO and Virgo detectors begin operation.http://journals.aps.org/prd/abstract/10.1103/PhysRevD.89.122004publishedVersionFil: Aasi, J. LIGO. California Institute of Technology; Estados Unidos de América.Fil: Domínguez, E. Argentinian Gravitational Wave Group; Argentina.Fil: Maglione, C. Argentinian Gravitational Wave Group; Argentina.Fil: Reula, O. Argentinian Gravitational Wave Group; Argentina.Fil: Ortega, W. Argentinian Gravitational Wave Group; Argentina.Fil: Wolovick, N. Argentinian Gravitational Wave Group; Argentina.Fil: Schilman, M. Argentinian Gravitational Wave Group; Argentina.Física de Partículas y Campo

Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

peer reviewe

Drawing Large Graphs by Multilevel Maxent-Stress Optimization

Drawing large graphs appropriately is an important step for the visual analysis of data from real-world networks. Here we present a novel multilevel algorithm to compute a graph layout with respect to a recently proposed metric that combines layout stress and entropy. As opposed to previous work, we do not solve the linear systems of the maxent-stress metric with a typical numerical solver. Instead we use a simple local iterative scheme within a multilevel approach. To accelerate local optimization, we approximate long-range forces and use shared-memory parallelism. Our experiments validate the high potential of our approach, which is particularly appealing for dynamic graphs. In comparison to the previously best maxent-stress optimizer, which is sequential, our parallel implementation is on average 30 times faster already for static graphs (and still faster if executed on one thread) while producing a comparable solution quality

Radio frequency identification (RFID) adoption: a cross-sectional comparison of voluntary and mandatory contexts

Understanding the adoption factors of a technological innovation is crucial. However, it is a wild assumption that these factors are of similar importance for mandatory and voluntary adoption. Hence, understanding the distinction is critical because, more than often an innovation is adopted with different organizational objectives—though operate in a same industry for a same application. The purpose of this study is to compare the organizational adoption factors of a technological innovation in mandatory and voluntary setting, taking Radio Frequency Identification (RFID) technology as the case innovation. The results indicate that perceptions of the adopters differ significantly on technological, organizational, and environmental characteristics and expectation when the contexts are different. Multi-group analysis confirms that, among the technological factors, compatibility is the major concern in amandatory setting whereas cost and expected-benefits are the main for voluntary adoption; organization’s attitude is more important than organizational resources—in both contexts;and, external pressure is important both in mandatory as well as voluntary environment

SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3

We present the results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments in 2009-2010, during the sixth LIGO science run and the second and third Virgo science runs. We perform two distinct searches: a modeled search for coalescences of either two neutron stars or a neutron star and black hole; and a search for generic, unmodeled gravitational-wave bursts. We find no evidence for gravitational-wave counterparts, either with any individual GRB in this sample or with the population as a whole. For all GRBs we place lower bounds on the distance to the progenitor, under the optimistic assumption of a gravitational-wave emission energy of 10^-2 M c^2 at 150 Hz, with a median limit of 17 Mpc. For short hard GRBs we place exclusion distances on binary neutron star and neutron star-black hole progenitors, using astrophysically motivated priors on the source parameters, with median values of 16 Mpc and 28 Mpc respectively. These distance limits, while significantly larger than for a search that is not aided by GRB satellite observations, are not large enough to expect a coincidence with a GRB. However, projecting these exclusions to the sensitivities of Advanced LIGO and Virgo, which should begin operation in 2015, we find that the detection of gravitational waves associated with GRBs will become quite possible.Comment: Accepted by ApJ. 19 pages, 8 figures, 2 tables, science summary page at http://www.ligo.org/science/Publication-S6GRB/index.php . Public access area to figures, tables at https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=p100012