10,827 research outputs found

    Theoretical Study of Fluid Forces on a Centrifugal Impeller Rotating and Whirling in a Volute

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    Fluid forces on a rotating and whirling centrifugal impeller in a volute are analyzed with the assumption of a two-dimensional rotational, inviscid flow. For simplicity, the flow is assumed to be perfectly guided by the impeller vanes. The theory predicts the tangential and the radial force on the whirling impeller as functions of impeller geometry, volute spacing, and whirl ratio. A good qualitative agreement with experiment is found

    Two-dimensional unsteady analysis of fluid forces on a whirling centrifugal impeller in a volute

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    Destabilizing fluid forces on a whirling centrifugal impeller rotating in a volute were observed. A quasisteady analysis neglecting shed vorticity or an unsteady analysis without a volute does not predict the existence of such destabilizing fluid forces on a whirling impeller. The effects of a volute and the shed vorticity are considered. We treat cases when an impeller with an infinite number of vanes rotates with a constant velocity omega and its center whirls with a constant eccentric radius epsilon and a constant whirling velocity psi. It is assumed that: (1) the number of the vanes is so large that the impeller can be treated as an actuator impeller in which the flow is perfectly guided; (2) flow is inviscid, incompressible and two dimensional; (3) the eccentricity epsilon is so small that unsteady components can be linearized; (4) vorticity is transported on a prescribed mean flow, the operating point is near design flow rate; and (5) the volute can be represented by a curved plate

    Ballistic Localization in Quasi-1D Waveguides with Rough Surfaces

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    Structure of eigenstates in a periodic quasi-1D waveguide with a rough surface is studied both analytically and numerically. We have found a large number of "regular" eigenstates for any high energy. They result in a very slow convergence to the classical limit in which the eigenstates are expected to be completely ergodic. As a consequence, localization properties of eigenstates originated from unperturbed transverse channels with low indexes, are strongly localized (delocalized) in the momentum (coordinate) representation. These eigenstates were found to have a quite unexpeted form that manifests a kind of "repulsion" from the rough surface. Our results indicate that standard statistical approaches for ballistic localization in such waveguides seem to be unappropriate.Comment: 5 pages, 4 figure

    A comparison of reflector antenna designs for wide-angle scanning

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    Conventional reflector antennas are typically designed for up to + or - 20 beamwidths scan. An attempt was made to stretch this scan range to some + or - 300 beamwidths. Six single and dual reflector antennas were compared. It is found that a symmetrical parabolic reflector with f/D = 2 and a single circular waveguide feed has the minimum scan loss (only 0.6 dB at Theta sub 0 = 8 deg, or a 114 beamwidths scan). The scan is achieved by tilting the parabolic reflector by an angle equal to the half-scan angle. The f/D may be shortened if a cluster 7 to 19 elements instead of one element is used for the feed. The cluster excitation is adjusted for each new beam scan direction to compensate for the imperfect field distribution over the reflector aperture. The antenna can be folded into a Cassegrain configuration except that, due to spillover and blockage considerations, the amount of folding achievable is small

    A comparison of reflector antenna designs for wide-angle scanning

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    Conventional reflector antennas are typically designed for up to + or - 20 beamwidths scan. An attempt was made to stretch this scan range to some + or - 300 beamwidths. Six single and dual reflector antennas were compared. It is found that a symmetrical parabolic reflector with f/D = 2 and a single circular waveguide feed has the minimum scan loss (only 0.6 dB at Theta sub 0 = 8 deg, or a 114 beamwidths scan). The scan is achieved by tilting the parabolic reflector by an angle equal to the half-scan angle. The f/D may be shortened if a cluster 7 to 19 elements instead of one element is used for the feed. The cluster excitation is adjusted for each new beam scan direction to compensate for the imperfect field distribution over the reflector aperture. The antenna can be folded into a Cassegrain configuration except that, due to spillover and blockage considerations, the amount of folding achievable is small

    Low optical polarisation at the core of the optically-thin jet of M87

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    We study the optical linear and circular polarisation in the optically-thin regime of the core and jet of M87. Observations were acquired two days before the Event Horizon Telescope (EHT) campaign in early April 2017. A high degree (20\sim 20 per cent) of linear polarisation (Plin_{\rm lin}) is detected in the bright jet knots resolved at 10arcsec\sim 10\, \rm{arcsec} to 23arcsec23\, \rm{arcsec} (0.80.8-1.8kpc1.8\, \rm{kpc}) from the centre, whereas the nucleus and inner jet show Plin5_{\rm lin} \lesssim 5 per cent. The position angle of the linear polarisation shifts by 90\sim 90 degrees from each knot to the adjacent ones, with the core angle perpendicular to the first knot. The nucleus was in a low level of activity (Plin2_{\rm lin} \sim 2-33 per cent), and no emission was detected from HST-1. No circular polarisation was detected either in the nucleus or the jet above a 3σ3\sigma level of Pcirc1.5_{\rm circ} \leq 1.5 per cent, discarding the conversion of Plin_{\rm lin} into Pcirc_{\rm circ}. A disordered magnetic field configuration or a mix of unresolved knots polarised along axes with different orientations could explain the low Plin_{\rm lin}. The latter implies a smaller size of the core knots, in line with current interferometric observations. Polarimetry with EHT can probe this scenario in the future. A steep increase of both Plin_{\rm lin} and Pcirc_{\rm circ} with increasing frequency is expected for the optically-thin domain, above the turnover point. This work describes the methodology to recover the four Stokes parameters using a λ/4\lambda/4 wave-plate polarimeter.Comment: Accepted for publication in MNRAS. 10 pages, 8 figure

    Assessing Electoral Personalism in Latin American Presidential Elections

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    Latin American democracies have been characterised as the product of personalistic leaders relying on their unique qualities to achieve and maintain political power. However, this characterisation has lacked conceptual and empirical development since the term “personalism” has been used to account simultaneously for a particular type of electoral appeal seeking to mobilise and persuade voters and for the concentration of power in a single political leader. This article advances in conceptualising electoral personalism as a strategy followed by political elites appealing to voters based on the personal characteristics of leaders and candidates, distinguishing it from personalisation as the concentration of power in a single leader. Based on statistical analysis, we propose two novel indicators of electoral personalism and assess its prevalence among Latin American countries. The article also advances in exploring its political, economic, and social determinants at the aggregate and individual levels.Agencia Nacional de Investigación e Innovació

    Mid-Infrared Images of Luminous Infrared Galaxies in a Merging Sequence

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    We report mid-infrared observations of several luminous infrared galaxies (LIGs) carried out with the Infrared Space Observatory. Our sample was chosen to represent different phases of a merger sequence of galaxy-galaxy interaction with special emphasis on early/intermediate stages of merging. The mid-infrared emission of these LIGs shows extended structures for the early and intermediate mergers, indicating that most of the mid-infrared luminosities are not from a central active galactic nucleus (AGN). Both the infrared hardness (indicated by the IRAS 12, 25, and 60 \micron flux density ratios) and the peak-to-total flux density ratios of these LIGs increase as projected separation of these interacting galaxies become smaller, consistent with increasing star formation activities that are concentrated to a smaller area as the merging process advances. These observations provide among the first observational constraint of largely theoretically based scenarios.Comment: 10 pages, 3 figures, please refer to ApJ Letters for the final versio

    Application of Near Infrared Reflectance Spectroscopy (NIRS) to Forage Evaluation in Uruguay

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    Near infrared reflectance spectroscopy (NIRS) were used to assess the chemical composition of a wide range of forages. Nearly five hundred herbage samples covering a wide range of temperate pastures species and mixtures, previously analysed by conventional wet chemistry were scanned in reflectance with a NIRS 6500 (NIRSystems, Silver Spring, USA). The coefficients of determination in calibration (R2 ) and the errors in cross validation (SECV) were 0.98 (5.8), 0.94 (22.2), 0.97 (5.6), 0.94 (6.9) and 0.89 (19.7) for crude protein, in vitro organic matter digestibility, dry matter, ash and acid detergent fiber, in g kg –1 on a dry weight respectively. The high correlation between NIRS and chemical analysis found in this study showed the potential use of NIRS for prediction forage quality
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