153,549 research outputs found

    Housing and council tax benefits administration in England: a long-term perspective on the performance of the local government delivery system

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    This paper evaluates the performance of the Council Tax and Housing Benefits Administration Services delivered by local authorities since the current system for the delivery of these benefits was introduced. During this period the performance of local government has been regulated and influenced by four successive national delivery regimes imposed by central governments namely Compulsory Competitive Tendering (CCT); Best Value (BV); Comprehensive Performance Assessments (CPA) and Comprehensive Area Assessments (CAA). An earlier paper (XXXX et al. forthcoming) examined the CPA period in detail and found a significant improvement in performance across all types of authorities in all parts of the country during this period. The current paper is intended to complement this earlier analysis and provide a longer term perspective on the performance of the benefits service under successive regimes between 1993 and 2010. The findings show that under CCT the performance of the system was poor, there were wide variations in individual local authority’s performance, with many acknowledged inadequacies in the system and unacceptably high levels of fraud. However in this period and in the subsequent BV period the antecedents of some of the tools and techniques subsequently used to drive improvement in the CPA era were either put in place or were being developed

    Comprehensive performance assessment and public services improvement in England? A case study of the benefits administration service in local government

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    The purpose of this paper is to independently evaluate the impact of the Comprehensive Performance Assessment regime on one particular public service, namely the provision of Council Tax and Housing Benefits distributed by local authorities throughout the course of the regime. This service was assessed in every iteration of the CPA methodologies and it included one of the few key performance indicators (KPIs) where the definition of the performance indicator, the means of collection and the public reporting of its results, remained the same throughout the CPA period between 2002 and 2008

    The applicability of MFD thrusters to satellite power systems

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    The high power self field MPD thruster uses electromagnetic forces rather than electrostatic to accelerate a neutral plasma. The most attractive application of MPD thrusters to satellite power systems is in the area of electric propulsion for a cargo orbit transfer vehicle (COTV). Calculations were performed in order to compare the performance of a COTV using an ion or MPD propulsion system. Results show that the MPD propulsion system gives a shorter trip time with the same power and payload when compared to the ion thruster propulsion system at either value of specific impulse. More important than the trip time benefit may be the advantage a MPD propulsion system provides in system simplicity. Another interesting COTV concept using MPD thrusters is the use of a remote power supply located on the Earth, at GEO, or somewhere in between to transmit power to the COTV in a microwave transmission. The specific impulse at thrust levels of tens of newtons makes a MPD propulsion system a candidate for stationkeeping and attitude control of large space structures such as a SPS

    A new effect in the low magnetic field ultrasonic attenuation of impure superconducting niobium

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    Low magnetic field ultrasonic attenuation of impure superconducting niobiu

    Cross-correlation of the unresolved X-ray background with faint galaxies

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    At the faint end of the deepest X-ray surveys, a population of X-ray luminous galaxies is seen. In this paper, we present the results of a cross-correlation between the residual, unresolved X-ray photons in a very deep X-ray survey and the positions of faint galaxies, in order to examine the importance of these objects at even fainter flux levels. We measure a significant correlation on all angular scales up to ~1 arcmin. This signal could account for a significant fraction of the unresolved X-ray background, approximately 35 per cent if the clustering is similar to optically selected galaxies. However, the angular form of the correlation is seen to be qualitatively similar to that expected for clusters of galaxies and the X-ray emission could be associated with hot gas in clusters or with QSOs within galaxy clusters rather than emission from individual faint galaxies. The relative contribution from each of these possibilities cannot be determined with the current data.Comment: 7 pages LaTeX including 9 EPS figures. Uses mn.sty. Accepted for publication by MNRA
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