23,398 research outputs found

    Inorganic thermal control pigment Patent

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    White paint production by heating impure aluminum silicate clay having low solar absorptanc

    Making physical education relevant: Increasing the impact of initial teacher training

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    This paper is developed from concern that, despite a number of developments and initiatives in physical education over recent years, there has been little change in the teaching of the subject. This has resulted in many young people being alienated from physical education and therefore physical activity. The paper focuses on how initial teacher training (ITT) contributes to this lack of change by focusing on the development of knowledge for teaching and the technical competence to deliver this. It then considers ways in which ITT could contribute to developing ‘knowledgeable teachers’ who are able to make change. The paper focuses on two aspects identified as relevant for trainee physical education teachers: socialisation and knowledge for teaching. It recognises that the issues are complex and that change is difficult. It also recognises that ITT cannot change things by itself. However, it argues that by maintaining the status quo, the subject will not develop so that it is relevant to today’s youngsters

    One application of mega-geomorphology in education

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    One advantage of a synoptic view displaying landform assemblages provided by imagery is that one can often identify geomorphic processes which have shaped the region and which may affect the habitability of the area over a human life time. Considering the continued growth of the world population and the resultant pressure and the exploitation of land, usually without any consideration given to geologic processes, it is imperative that we attempt to educate as large a segment of the population as we can about geologic processes and how they influence land use. Space platform imagery which exhibits regional landscapes can be used: (1) to show students the impact of geologic processes over relatively short periods of time (e.g., the Mount St. Helens lateral blast); (2) to display the effects of poor planning because of a lack of knowledge of the local geologic processes (e.g., the 1973 image of the Mississippi River flood around St. Louis, MO); and (3) to show the association of certain types of landforms with building materials and other resources (e.g., drumlins and gravel deposits)

    Measurement of airfoil heat transfer coefficients on a turbine stage

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    The primary basis for heat transfer analysis of turbine airfoils is experimental data obtained in linear cascades. A detailed set of heat transfer coefficients was obtained along the midspan of a stator and a rotor in a rotating turbine stage. The data are to be compared to standard analyses of blade boundary layer heat transfer. A detailed set of heat transfer coefficients was obtained along the midspan of a stator located in the wake of a full upstream turbine stage. Two levels of inlet turbulence (1 and 10 percent) were used. The analytical capability will be examined to improve prediction of the experimental data

    Digital multishaker modal testing

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    A review of several modal testing techniques is made, along with brief discussions of their advantages and limitations. A new technique is presented which overcomes many of the previous limitations. Several simulated experiments are included to verify the validity and accuracy of the new method. Conclusions are drawn from the simulation studies and recommendations for further work are presented. The complete computer code configured for the simulation study is presented

    B-Physics at the Tevatron (Proceedings of PASCOS2010)

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    We report on recent B-Physics results from the Tevatron. The topics covered include measurement of the polarization amplitudes in Bs0→ϕϕB_s^0 \to \phi \phi, the search for rare flavor-changing neutral-current decays, CP violation in Bs0→J/ψϕB_s^0 \to J/\psi \phi and semileptonic Bs0B_s^0 decays, and a new measurement of the like-sign asymmetry in dimuon events.Comment: 6 pages, proceedings paper, 16th International Symposium on Particles, Strings, and Cosmology, Valencia, Spain, July 19 - 23, 201

    Using temporal distributions of transient events to characterize cosmological source populations

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    The brightest events in a time series of cosmological transients obey an observation time dependence which is often overlooked. This dependence can be exploited to probe the global properties of electromagnetic and gravitational wave transients (Howell et al. 2007a, Coward & Burman 2005). We describe a new relation based on a peak flux--observation time distribution and show that it is invariant to the luminosity distribution of the sources (Howell et al. 2007b). Applying this relation, in combination with a new data analysis filter, to \emph{Swift} gamma-ray burst data, we demonstrate that it can constrain their rate density.Comment: published in proceedings of FRONTIERS OF FUNDAMENTAL AND COMPUTATIONAL PHYSICS: 10th International Symposium, AIP,1246,203, (2010

    An improved method for estimating source densities using the temporal distribution of Cosmological Transients

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    It has been shown that the observed temporal distribution of transient events in the cosmos can be used to constrain their rate density. Here we show that the peak flux--observation time relation takes the form of a power law that is invariant to the luminosity distribution of the sources, and that the method can be greatly improved by invoking time reversal invariance and the temporal cosmological principle. We demonstrate how the method can be used to constrain distributions of transient events, by applying it to Swift gamma-ray burst data and show that the peak flux--observation time relation is in good agreement with recent estimates of source parameters. We additionally show that the intrinsic time dependence allows the method to be used as a predictive tool. Within the next year of Swift observation, we find a 50% chance of obtaining a peak flux greater than that of GRB 060017 -- the highest Swift peak flux to date -- and the same probability of detecting a burst with peak flux > 100 photons s^{-1} cm^{-2} within 6 years.Comment: Submitted to ApJ Letter
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