26,500 research outputs found

    Supersonic fan blading

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    Radially extending rotor blades are disposed on a hub to form a supersonic propulsion fan for a turbofan engine. The peripheral spacing of the blades is such as to avoid forming a channel or passageway between adjacent blades. Each has a flat trailing surface extending from the leading edge at least as far to the rear as to cause any pressure waves which might originate on the blade surface to strike the leading surface of the following blade rather than propagate upstream of the blade row. The flat trailing surface of each blade makes an angle with the axis of rotation such that the blade is parallel to a gas inflow into the blades

    Acoustic properties of a supersonic fan

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    Acoustic properties of supersonic fan with short blade spa

    Densities and abundances of hot cometary ions in the coma of P/Halley

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    On its flight by P/Halley, the Giotto spacecraft carried a High Energy Range Spectrometer (HERS) for measuring the properties of cometary ions picked up by the solar wind in the nearly collisionless regions of the coma. Preliminary estimates of the ion densities observed by HERS were reevaluated and extended; density profiles along the Giotto trajectory are presented for 13 values of ion mass/charge. Comparison with the physical-chemical model of the interaction of sunlight and the solar wind with the comet by other researchers reveals that, with the exception of protons and H2(+), all ion densities were at least an order of magnitude higher than predicted. The high ion densities cannot be explained on the basis of compression of the plasma, but require additional or stronger ionization mechanisms. Ratios of the densities of different ion species reveal an overabundance of carbonaceous material and an underabundance of H2(+) compared to the predictions of the Schmidt. While the densities of solar wind ions (H(+) and He(++)) changed sharply across a magnetic discontinuity located 1.35(10)(exp 5) km from the comet, this feature, which has been called both the 'cometopause' and the 'magnetic pileup boundary' was barely distinguishable in the density profiles of hot cometary ions. This result is consistent with the interpretation that the magnetic pileup boundary detected by Giotto was caused by a discontinuity in the solar wind and is not an intrinsic feature of the interaction of the solar wind with an active comet

    Influence of environmental factors during seed development and after full-ripeness on pre-harvest sprouting in wheat

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    Results on environmental and genotypic factors influencing preharvest sprouting of wheat are summarized. Other possible areas where additional research is needed is suggested

    Performance of a straight stator and a tilted stator tested with a high-solidity high-pressure-ratio transonic rotor

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    Overall stage and stator blade element performance with straight stator and tilted stator in transonic axial flow compressor stag

    Triangular buckling patterns of twisted inextensible strips

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    When twisting a strip of paper or acetate under high longitudinal tension, one observes, at some critical load, a buckling of the strip into a regular triangular pattern. Very similar triangular facets have recently been observed in solutions to a new set of geometrically-exact equations describing the equilibrium shape of thin inextensible elastic strips. Here we formulate a modified boundary-value problem for these equations and construct post-buckling solutions in good agreement with the observed pattern in twisted strips. We also study the force-extension and moment-twist behaviour of these strips by varying the mode number n of triangular facets

    Celestial mechanics in Kerr spacetime

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    The dynamical parameters conventionally used to specify the orbit of a test particle in Kerr spacetime are the energy EE, the axial component of the angular momentum, LzL_{z}, and Carter's constant QQ. These parameters are obtained by solving the Hamilton-Jacobi equation for the dynamical problem of geodesic motion. Employing the action-angle variable formalism, on the other hand, yields a different set of constants of motion, namely, the fundamental frequencies ωr\omega_{r}, ωθ\omega_{\theta} and ωϕ\omega_{\phi} associated with the radial, polar and azimuthal components of orbital motion. These frequencies, naturally, determine the time scales of orbital motion and, furthermore, the instantaneous gravitational wave spectrum in the adiabatic approximation. In this article, it is shown that the fundamental frequencies are geometric invariants and explicit formulas in terms of quadratures are derived. The numerical evaluation of these formulas in the case of a rapidly rotating black hole illustrates the behaviour of the fundamental frequencies as orbital parameters such as the semi-latus rectum pp, the eccentricity ee or the inclination parameter θ−\theta_{-} are varied. The limiting cases of circular, equatorial and Keplerian motion are investigated as well and it is shown that known results are recovered from the general formulas.Comment: 25 pages (LaTeX), 5 figures, submitted to Class. Quantum Gra

    Silphium Perfoliatum: A North American Prairie Plant with Potential as a Forage Crop

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    Cup-plant (Silphium perfoliatum L.) is a perennial member of the Asteraceae family, native to mesic sites of the North American prairie. Two experiments were conducted to gain knowledge of the performance of cup-plant grown in monoculture as a managed, harvested crop. In the first experiment, three cup-plant ecotypes grown near East Troy, WI and harvested twice per season for 3 years yielded from 9 to 11 Mg ha-1 each season. Mean neutral detergent fiber concentration was 385 g kg-1, acid detergent fiber 290 g kg-1, and crude protein 175 g kg-1 at late bud. The second experiment was an evaluation of performance of 28 ecotypes at three locations in Wisconsin. The mean performance was similar to the first experiment, however there was substantial variation for yield, forage quality, and pest resistance among the lines evaluated. We conclude that cup-plant has potential as a forage crop in temperate regions of the world, and that some ecotypes exhibit superior performance
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