292 research outputs found

    Control of inverter-based micro-grids

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    Control and filter design of three-phase inverters for high power quality grid connection

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    Dynamic Stability of a Microgrid With an Active Load

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    High-quality power generation through distributed control of a power park microgrid

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    Interaction design for rural agricultural sensor networks

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    We describe the ongoing design of a sensor network for small family farms in rural Kenya. The sensor network is just one part of an ‘ecology of resources’ in which handheld devices are used to bridge the sensor network and a computer-based access point. We describe the two villages where the system is deployed and the user requirements collected. We then describe the architecture of the sensor network and detail how it fits in with the larger integrated system. We then detail our approach to interface and interaction design, and conclude by describing the next steps in the project

    A Bitter Pill: The Primordial Lithium Problem Worsens

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    The lithium problem arises from the significant discrepancy between the primordial 7Li abundance as predicted by BBN theory and the WMAP baryon density, and the pre-Galactic lithium abundance inferred from observations of metal-poor (Population II) stars. This problem has loomed for the past decade, with a persistent discrepancy of a factor of 2--3 in 7Li/H. Recent developments have sharpened all aspects of the Li problem. Namely: (1) BBN theory predictions have sharpened due to new nuclear data, particularly the uncertainty on 3He(alpha,gamma)7Be, has reduced to 7.4%, and with a central value shift of ~ +0.04 keV barn. (2) The WMAP 5-year data now yields a cosmic baryon density with an uncertainty reduced to 2.7%. (3) Observations of metal-poor stars have tested for systematic effects, and have reaped new lithium isotopic data. With these, we now find that the BBN+WMAP predicts 7Li/H = (5.24+0.71-0.67) 10^{-10}. The Li problem remains and indeed is exacerbated; the discrepancy is now a factor 2.4--4.3 or 4.2sigma (from globular cluster stars) to 5.3sigma (from halo field stars). Possible resolutions to the lithium problem are briefly reviewed, and key nuclear, particle, and astronomical measurements highlighted.Comment: 21 pages, 4 figures. Comments welcom
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