8,937 research outputs found

    Systems, interactions and macrotheory

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    A significant proportion of early HCI research was guided by one very clear vision: that the existing theory base in psychology and cognitive science could be developed to yield engineering tools for use in the interdisciplinary context of HCI design. While interface technologies and heuristic methods for behavioral evaluation have rapidly advanced in both capability and breadth of application, progress toward deeper theory has been modest, and some now believe it to be unnecessary. A case is presented for developing new forms of theory, based around generic “systems of interactors.” An overlapping, layered structure of macro- and microtheories could then serve an explanatory role, and could also bind together contributions from the different disciplines. Novel routes to formalizing and applying such theories provide a host of interesting and tractable problems for future basic research in HCI

    Building relationships with the invisible in the digital (global) economy (BRIDGE).

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    Access to products, services and government is increasingly reliant on people being able to use information and communications technologies: from computers to mobile phones. Whilst there are many obvious benefits to those already familiar with the technology, those that do not have the skills or inclination to interact through such technology can get excluded and this may eventually lead to a permanent disadvantage. These groups within society can be very large according to the UK government, with 70% of over 65s reported as never having used the Internet (www.statistics.gov.uk, 2008). As companies grow in scale and design products and services for global rather than local markets it becomes harder to track these partially excluded groups. This is reported as a growing 'psychic distance' between the designers of technologies and the prospective users of those technologies, with a risk that those excluded from the market today will become effectively invisible to designers of future products. Such users' requirements of technology no longer inform the design process and create a digital divide that is socially constructed rather than economically constrained. This is neither good for society nor business, where such exclusion may alienate, as well as prevent business from identifying and engaging with latent demand for their products and services. This project aims to build a 'Bridge' from the needs of technologically excluded users to the capabilities of suppliers of products and services. This will be achieved through exploration of users' expectations, desires and needs and by building design guidelines to help address them. The project will extrapolate the results of this work to wider markets. In order to realise these goals, a combination is needed of qualitative research methods to deliver a detailed picture of user needs, and quantitative methods to map that to the data that large global corporations would typically hold about their current customers and markets. User needs identified through qualitative methods need to be related to behavioural characteristics observed through data analysis and modelling of demand within global markets. This element of the project builds on direct engagement with industry, both with designers, and their existing customers, as well as the organisational processes and data that relate one to the other and informs the designer's view of their users. Through direct engagement with users, designers and producers, BRIDGE will contribute to the design of new products, services and interfaces. As design improves and becomes more socially inclusive, better and more sustainable relationships can be established with consumers. This knowledge can be used to identify opportunities for expansion within global markets for UK industry and hence has the potential to benefit individuals, society and the economy overall

    The Distribution of X-ray Dips with Orbital Phase in Cygnus X-1

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    We present results of a comprehensive study of the distribution of absorption dips with orbital phase in Cygnus X-1. Firstly, the distribution was obtained using archival data from all major X-ray observatories and corrected for the selection effect that phase zero (superior conjunction of the black hole) has been preferentially observed. Dip occurrence was seen to vary strongly with orbital phase \phi, with a peak at \phi ~ 0.95, i.e. was not symmetric about phase zero. Secondly, the RXTE ASM has provided continuous coverage of the Low State of Cygnus X-1 since Sept. 1996, and we have selected dip data based on increases in hardness ratio. The distribution, with much increased numbers of dip events, confirms that the peak is at \phi ~ 0.95, and we report the discovery of a second peak at \phi ~ 0.6. We attribute this peak to absorption in an accretion stream from the companion star HDE 226868. We have estimated the ionization parameter at different positions showing that radiative acceleration of the wind is suppressed by photoionization in particular regions in the binary system. To obtain the variation of column density with phase, we make estimates of neutral wind density for the extreme cases that acceleration of the wind is totally suppressed, or not suppressed at all. An accurate description will lie between these extremes. In each case, a strong variation of column density with orbital phase resulted, similar to the variation of dip occurrence. This provides evidence that formation of the blobs in the wind which lead to absorption dips depends on the density of the neutral component in the wind, suggesting possible mechanisms for blob growth.Comment: 9 pages, Latex, 7 ps figures. accepted by MNRA

    City of Hampton Tidal Marsh Inventory

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    Exploring Parameter Constraints on Quintessential Dark Energy: The Exponential Model

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    We present an analysis of a scalar field model of dark energy with an exponential potential using the Dark Energy Task Force (DETF) simulated data models. Using Markov Chain Monte Carlo sampling techniques we examine the ability of each simulated data set to constrain the parameter space of the exponential potential for data sets based on a cosmological constant and a specific exponential scalar field model. We compare our results with the constraining power calculated by the DETF using their ``w0−waw_0-w_a'' parametrization of the dark energy. We find that respective increases in constraining power from one stage to the next produced by our analysis give results consistent with DETF results. To further investigate the potential impact of future experiments, we also generate simulated data for an exponential model background cosmology which can not be distinguished from a cosmological constant at DETF ``Stage 2'', and show that for this cosmology good DETF Stage 4 data would exclude a cosmological constant by better than 3σ\sigma.Comment: 11 pages including 10 figure
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