7,322 research outputs found

    Study of an advanced transport airplane design concept known as Flatbed

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    The design concept and configuration of the Flatbed transport aircraft are presented. The Flatbed configuration combines into one frame, the ability to haul cargo, virtually unrestrained by cross sectional dimensions of the fuselage. The feasibility and capability of the Flatbed is discussed in depth

    Simulation Of Human Jumping - Task Alteration

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    Similar human motions are often grouped together into a single movement class. In jumping, the question of similarity in control and coordination of different tasks within a movement class has been addressed by altering the direction of maximal effort jumps between vertical and horizontal (Jensen & Phillips, 1991). Other researchers have studied vertical jumping using computer simulations (Pandy & Zajac, 1991; van Soest et al., 1993), but have not addressed the issue of modifying the jumping task. The purpose of the present study was to investigate the effect of task alteration on forward .dynamic simulations of jumping. The simulation model was comprised of 4 linked rigid segments (Fig. 1). Segmental motion was controlled by 3 torque generators defined with pre-set magnitudes and activation time constants. All jumps began from a static posture with all torques set to zero. Each jumping performance was dictated by the onset times of each torque generator. The choice of task was specified by one of two objective functions: 1) vertical height, or 2) horizontal distance. The optimization algorithm searched for the pattern of activation onset times for the 3 torque generators which maximized each objective function. A variety of tests were performed to compare the model's optimal vertical and horizontal jumping performance, and the underlying coordination of torque generation. With the set of initial conditions shown in Fig. la (00 = (1.0,-0.7,1.1,-0.8}), the model's maximum height was 1.814 m, with a forward displacement of 0.39 m. For the optimal forward jump the displacement increased to only 0.73 m. However, by changing the initial posture (00 = (0.8,-1.0,0.8,-1.0}) the optimal forward jump was improved to 1.87 m (Fig. lb), but the optimal vertical jump was reduced to 1.465 m. The relative magnitude of onset times varied substantially between the two optimal jumps. For the conditions studied, the order of onset times does not follow the proximo-distal sequence often .proported for humans, and the relative timing of joint torques changes with task. The results illustrate the dependence of the optimal solution on initial conditions. Further work will examine the relations between initial conditions, coordination and perfommance

    Collapse of a Circular Loop of Cosmic String

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    We study the collapse of a circular loop of cosmic string. The gravitational field of the string is treated using the weak field approximation. The gravitational radiation from the loop is evaluated numerically. The memtric of the loop near the point of collapse is found analytically.Comment: 15 page

    Exploring the Chemical Composition and Double Horizontal Branch of the Bulge Globular Cluster NGC 6569

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    Photometric and spectroscopic analyses have shown that the Galactic bulge cluster Terzan 5 hosts several populations with different metallicities and ages that manifest as a double red horizontal branch (HB). A recent investigation of the massive bulge cluster NGC 6569 revealed a similar, though less extended, HB luminosity split, but little is known about the cluster's detailed chemical composition. Therefore, we have used high-resolution spectra from the Magellan-M2FS and VLT-FLAMES spectrographs to investigate the chemical compositions and radial velocity distributions of red giant branch and HB stars in NGC 6569. We found the cluster to have a mean heliocentric radial velocity of -48.8 km/s (sigma = 5.3 km/s; 148 stars) and a mean [Fe/H] =-0.87 dex (19 stars), but the cluster's 0.05 dex [Fe/H] dispersion precludes a significant metallicity spread. NGC 6569 exhibits light- and heavy-element distributions that are common among old bulge/inner Galaxy globular clusters, including clear (anti)correlations between [O/Fe], [Na/Fe], and [Al/Fe]. The light-element data suggest that NGC 6569 may be composed of at least two distinct populations, and the cluster's low mean [La/Eu] = -0.11 dex indicates significant pollution with r-process material. We confirm that both HBs contain cluster members, but metallicity and light-element variations are largely ruled out as sources for the luminosity difference. However, He mass fraction differences as small as delta Y ~ 0.02 cannot be ruled out and may be sufficient to reproduce the double HB.Comment: 72 pages, 14 figures, 8 tables; published in The Astronomical Journal; electronic versions of all tables are available in the published versio

    Anisotropy of the Cosmic Neutrino Background

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    The cosmic neutrino background (CNB) consists of low-energy relic neutrinos which decoupled from the cosmological fluid at a redshift z ~ 10^{10}. Despite being the second-most abundant particles in the universe, direct observation remains a distant challenge. Based on the measured neutrino mass differences, one species of neutrinos may still be relativistic with a thermal distribution characterized by the temperature T ~ 1.9K. We show that the temperature distribution on the sky is anisotropic, much like the photon background, experiencing Sachs-Wolfe and integrated Sachs-Wolfe effects.Comment: 5 pages, 2 figures / updated references, discussion of earlier wor

    Nucleating Black Holes via Non-Orientable Instantons

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    We extend the analysis of black hole pair creation to include non- orientable instantons. We classify these instantons in terms of their fundamental symmetries and orientations. Many of these instantons admit the pin structure which corresponds to the fermions actually observed in nature, and so the natural objection that these manifolds do not admit spin structure may not be relevant. Furthermore, we analyse the thermodynamical properties of non-orientable black holes and find that in the non-extreme case, there are interesting modifications of the usual formulae for temperature and entropy.Comment: 27 pages LaTeX, minor typos are correcte

    The Lower Carboniferous rocks of the Carrick Syncline

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