1,268 research outputs found

    Design description of the Schuchuli Village photovoltaic power system

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    A stand alone photovoltaic (PV) power system for the village of Schuchuli (Gunsight), Arizona, on the Papago Indian Reservation is a limited energy, all 120 V (d.c.) system to which loads cannot be arbitrarily added and consists of a 3.5 kW (peak) PV array, 2380 ampere-hours of battery storage, an electrical equipment building, a 120 V (d.c.) electrical distribution network, and equipment and automatic controls to provide control power for pumping water into an existing water system; operating 15 refrigerators, a clothes washing machine, a sewing machine, and lights for each of the homes and communal buildings. A solar hot water heater supplies hot water for the washing machine and communal laundry. Automatic control systems provide voltage control by limiting the number of PV strings supplying power during system operation and battery charging, and load management for operating high priority at the expense of low priority loads as the main battery becomes depleted

    Operational performance of the photovoltaic-powered grain mill and water pump at Tangaye, Upper Volta

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    The first two years of operation of a stand alone photovoltaic (PV) power system for the village of Tangaye, Upper Volta in West Africa are described. The purpose of the experiment was to demonstrate that PV systems could provide reliable electrical power for multiple use applications in remote areas where local technical expertise is limited. The 1.8 kW (peak) power system supplies 120-V (d.c.) electrical power to operate a grain mill, a water pump, and mill building lights for the village. The system was initially sized to pump a part of the village water requirements from an existing improved well, and to meet a portion of the village grain grinding requirements. The data, observations, experiences, and conclusions developed during the first two years of operation are discussed. Reports of tests of the mills used in the project are included

    Tunisia Renewable Energy Project systems description report

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    In 1979, the Agency for International Development (AID) initiated a renewable energy project with the Government of Tunisia to develop an institutional capability to plan and institute renewable energy technologies in a rural area. The specific objective of the district energy applications subproject was to demonstrate solar and wind energy systems in a rural village setting. The NASA Lewis Research Center was asked by the AID Near East Bureau to manage and implement this subproject. This report describes the project and gives detailed desciptions of the various systems

    Do the adult daughters of PCOS patients develop PCOS and is this due to an androgenized uterine environment-an online epidemiological survey

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    Objectives: Several inconsistent studies have investigated whether the uterine environment of androgenized pregnant women is a risk factor for an in-utero developmental imprinted predisposition towards subsequent polycystic ovarian syndrome (PCOS) among their female offspring. These are difficult to compare due to variable parameters and subject selection criteria. Few epidemiological studies have analyzed the incidence of PCOS amongst adult daughters of PCOS affected women previously. Our study aimed to investigate risk factors relating to the development of PCOS in the female offspring of PCOS patients. Methods: We used a questionnaire to collect a mother-to-daughter medical history and relevant information, in order to understand risk factors, which might relate to the presence of PCOS daughters of PCOS patients. Results: Of four hundred and one responses, 131 participants were included in the final analysis. There was no statistical association with the subsequent development of PCOS amongst female offspring of women with PCOS. However, there was a significantly higher prevalence of post-term birth among PCOS mothers. Nevertheless, the major determinant of risk of subsequent incidence of PCOS amongst daughters was a higher BMI, regardless of the mothers BMI. Conclusion: Socio-economic family influences, affecting BMI, may be the reason for any mother to daughter association with PCOS

    Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue - VI. AK Fornacis - a rare, bright K-type eclipsing binary

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    We present the results of the combined photometric and spectroscopic analysis of a bright (V=9.14), nearby (d=31 pc), late-type detached eclipsing binary AK Fornacis. This P=3.981 d system has not been previously recognised as a double-lined spectroscopic binary, and this is the first full physical model of this unique target. With the FEROS, CORALIE and HARPS spectrographs we collected a number of high-resolution spectra in order to calculate radial velocities of both components of the binary. Measurements were done with our own disentangling procedure and the TODCOR technique, and were later combined with the photometry from the ASAS and SuperWASP archives. We also performed an atmospheric analysis of the component spectra with the Spectroscopy Made Easy (SME) package. Our analysis shows that AK For consists of two active, cool dwarfs having masses of M1=0.6958±0.0010M_1=0.6958 \pm 0.0010 and M2=0.6355±0.0007M_2=0.6355 \pm 0.0007 M⊙_\odot and radii of R1=0.687±0.020R_1=0.687 \pm 0.020 and R2=0.609±0.016R_2=0.609 \pm 0.016 R⊙_\odot, slightly less metal abundant than the Sun. Parameters of both components are well reproduced by the models. AK For is the brightest system among the known eclipsing binaries with K or M type stars. Its orbital period is one of the longest and rotational velocities one of the lowest, which allows us to obtain very precise radial velocity measurements. The precision in physical parameters we obtained places AK For among the binaries with the best mass measurements in the literature. It also fills the gap in our knowledge of stars in the range of 0.5-0.8 M⊙_\odot, and between short and long-period systems. All this makes AK For a unique benchmark for understanding the properties of low-mass stars.Comment: 9 pages, 11 figures, 3 tables, accpeted for publication in A&
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