5,886 research outputs found

    Outcome of pregnancy in diabetic women

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    Development of a simulation-based decision support tool for renewable energy integration and demand-supply matching

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    This paper describes a simulation-based decision support tool, MERIT, which has been developed to assist in the assessment of renewable energy systems by focusing on the degree of match achievable between energy demand and supply. Models are described for the prediction of the performance of PV, wind and battery technologies. These models are based on manufacturers' specifications, location-related parameters and hourly weather data. The means of appraising the quality of match is outlined and examples are given of the application of the tool at the individual building and community levels

    Development and demonstration of a renewable energy based demand/supply decision support tool for the building design profession

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    Future cities are likely to be characterised by a greater level of renewable energy systems deployment. Maximum impact will be achieved when such systems are used to offset local energy demands in contrast to current philosophy dictating the grid connection of large schemes. This paper reports on the development of a software tool, MERIT, for demand/ supply matching. The purpose of MERIT is to assist with the deployment of renewable energy systems at all scales. This paper describes the procedures used to match heterogeneous supply technologies to a set of demand profiles corresponding to the different possible fuel types

    On the fidelity of the core mass functions derived from dust column density data

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    Aims: We examine the recoverability and completeness limits of the dense core mass functions (CMFs) derived for a molecular cloud using extinction data and a core identification scheme based on two-dimensional thresholding. Methods: We performed simulations where a population of artificial cores was embedded into the variable background extinction field of the Pipe nebula. We extracted the cores from the simulated extinction maps, constructed the CMFs, and compared them to the input CMFs. The simulations were repeated using a variety of extraction parameters and several core populations with differing input mass functions and differing degrees of crowding. Results: The fidelity of the observed CMF depends on the parameters selected for the core extraction algorithm for our background. More importantly, it depends on how crowded the core population is. We find that the observed CMF recovers the true CMF reliably when the mean separation of cores is larger than their mean diameter (f>1). If this condition holds, the derived CMF is accurate and complete above M > 0.8-1.5 Msun, depending on the parameters used for the core extraction. In the simulations, the best fidelity was achieved with the detection threshold of 1 or 2 times the rms-noise of the extinction data, and with the contour level spacings of 3 times the rms-noise. Choosing larger threshold and wider level spacings increases the limiting mass. The simulations show that when f>1.5, the masses of individual cores are recovered with a typical uncertainty of 25-30 %. When f=1 the uncertainty is ~60 %. In very crowded cases where f<1 the core identification algorithm is unable to recover the masses of the cores adequately. For the cores of the Pipe nebula f~2.0 and therefore the use of the method in that region is justified.Comment: 9 pages, 6 figures, accepted for publication in A&

    A Physical Limit to the Magnetic Fields of T Tauri Stars

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    Recent estimates of magnetic field strengths in T Tauri stars yield values B=1B=1--4 kG4\,{\rm kG}. In this paper, I present an upper limit to the photospheric values of BB by computing the equipartition values for different surface gravities and effective temperatures. The values of BB derived from the observations exceed this limit, and I examine the possible causes for this discrepancy

    Merit - An evaluation tool for 100% renewable energy provision

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    Islands represent an interesting challenge in terms of energy supply. A great deal of work has been carried out to look at specific aspects of this issue on different islands. Unfortunately, results from one study cannot be easily applied to other islands due to island-specific resources and energy-use profiles. A quantitative evaluation tool (MERIT) is presented here, which is able to match half-hourly energy demands (heat, electricity, hot water and transport) with local supplies. The program examines the energy balance on any scale, from an individual building through to an entire country, thereby providing a powerful and generic aid to decision making. This paper demonstrates the generality and usefulness of MERIT by using it to analyse the options for creating an energy-autonomous community on a typical, small island off the west coast of Scotland. Results are presented showing the feasibility of accomplishing 100% renewable provision on this island using available local resources

    The effect of a strong external radiation field on protostellar envelopes in Orion

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    We discuss the effects of an enhanced interstellar radiation field (ISRF) on the observables of protostellar cores in the Orion cloud region. Dust radiative transfer is used to constrain the envelope physical structure by reproducing SCUBA 850 micron emission. Previously reported 13CO, C17O and H2CO line observations are reproduced through detailed Monte Carlo line radiative transfer models. It is found that the 13CO line emission is marginally optically thick and sensitive to the physical conditions in the outer envelope. An increased temperature in this region is needed in order to reproduce the 13CO line strengths and it is suggested to be caused by a strong heating from the exterior, corresponding to an ISRF in Orion 10^3 times stronger than the "standard" ISRF. The typical temperatures in the outer envelope are higher than the desorption temperature for CO. The C17O emission is less sensitive to this increased temperature but rather traces the bulk envelope material. The data are only fit by a model where CO is depleted, except in the inner and outermost regions where the temperature increases above 30-40 K. The fact that the temperatures do not drop below approximately 25 K in any of the envelopes whereas a significant fraction of CO is frozen-out suggest that the interstellar radiation field has changed through the evolution of the cores. The H2CO lines are successfully reproduced in the model of an increased ISRF with constant abundances of 3-5x10^{-10}.Comment: 11 pages, 10 figures. Accepted for publication in A&

    Environmental Conditions and Vegetation Recovery at Abandoned Drilling Mud Sumps in the Mackenzie Delta Region, Northwest Territories, Canada

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    Historical data from oil and gas exploration in the delta of the Mackenzie River, Northwest Territories, in the 1970s provided an opportunity to estimate decadal-scale impacts of exploratory oil and gas drilling on native plant communities in low Arctic tundra. We assessed changes in vegetation composition and associated environmental gradients across seven drilling mud sumps in the Kendall Island Bird Sanctuary, Mackenzie Delta. Three decades after disturbance, drilling sumps had developed vegetation coverage equivalent to that in undisturbed areas, although bare soil persisted in ponded areas and where a salt crust was present. Vegetation on sumps was composed of communities dominated by forbs, grasses, and tall shrubs that were distinct from adjacent, undisturbed sedge and low shrub communities. The area of altered vegetation around a sump was generally larger in upland or saline environments than in lowland areas. Pooled water observed around many sumps was likely associated with thaw subsidence that occurred following construction, which was subsequently compounded by snow drifting and increased soil temperatures along the margins of the sump mound. Changes in drainage, active-layer depth, and surface salt concentrations appear to be key environmental factors that have helped shape plant communities established on drilling sumps in the three decades after disturbance.Les donnĂ©es historiques relatives Ă  l’exploration pĂ©troliĂšre et gaziĂšre rĂ©alisĂ©e dans le delta du fleuve Mackenzie, Territoires du Nord-Ouest, dans les annĂ©es 1970 ont permis d’estimer les incidences dĂ©cadaires des forages pĂ©troliers et gaziers exploratoires sur les peuplements de vĂ©gĂ©taux rĂ©gionaux de la basse toundra arctique. Nous avons Ă©valuĂ© les changements caractĂ©risant la composition de la vĂ©gĂ©tation et les gradients environnementaux connexes relativement Ă  sept bassins Ă  boue du refuge d’oiseaux de l’üle Kendall, dans le delta du Mackenzie. Trois dĂ©cennies aprĂšs la perturbation, la couverture vĂ©gĂ©tale des bassins Ă  boue Ă©tait Ă©quivalente Ă  celle des endroits non perturbĂ©s, bien qu’il restait toujours du sol dĂ©nudĂ© dans les endroits en prĂ©sence d’étangs et de croĂ»tes salĂ©es. Le vĂ©gĂ©tation se retrouvant sur les bassins Ă©tait composĂ©e d’herbes non graminĂ©ennes, de graminĂ©es et de grands arbrisseaux diffĂ©rents des peuplements adjacents constituĂ©s de laiche et de petits arbrisseaux non perturbĂ©s. La zone caractĂ©risĂ©e par la nouvelle vĂ©gĂ©tation autour d’un bassin Ă©tait gĂ©nĂ©ralement plus volumineuse dans les hautes terres ou les milieux salins que dans les basses terres. L’eau accumulĂ©e autour de nombreux bassins dĂ©coulait vraisemblablement de la subsidence attribuable au dĂ©gel qui s’est manifestĂ© aprĂšs la construction, ce qui a Ă©tĂ© aggravĂ© par la poudrerie et les tempĂ©ratures du sol Ă  la hausse le long des marges du monticule des bassins. Les changements en matiĂšre de ruissellement, de profondeur de la couche active et de concentrations de sel de surface semblent constituer d’importants facteurs environnementaux ayant aidĂ© Ă  façonner les peuplements de vĂ©gĂ©taux qui se sont Ă©tablis sur les bassins de forage au cours des trois dĂ©cennies ayant suivi la perturbation
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