719 research outputs found

    Effects of errorless learning on the acquisition of velopharyngeal movement control

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    Session 1pSC - Speech Communication: Cross-Linguistic Studies of Speech Sound Learning of the Languages of Hong Kong (Poster Session)The implicit motor learning literature suggests a benefit for learning if errors are minimized during practice. This study investigated whether the same principle holds for learning velopharyngeal movement control. Normal speaking participants learned to produce hypernasal speech in either an errorless learning condition (in which the possibility for errors was limited) or an errorful learning condition (in which the possibility for errors was not limited). Nasality level of the participants’ speech was measured by nasometer and reflected by nasalance scores (in %). Errorless learners practiced producing hypernasal speech with a threshold nasalance score of 10% at the beginning, which gradually increased to a threshold of 50% at the end. The same set of threshold targets were presented to errorful learners but in a reversed order. Errors were defined by the proportion of speech with a nasalance score below the threshold. The results showed that, relative to errorful learners, errorless learners displayed fewer errors (50.7% vs. 17.7%) and a higher mean nasalance score (31.3% vs. 46.7%) during the acquisition phase. Furthermore, errorless learners outperformed errorful learners in both retention and novel transfer tests. Acknowledgment: Supported by The University of Hong Kong Strategic Research Theme for Sciences of Learning © 2012 Acoustical Society of Americapublished_or_final_versio

    NASA SBIR abstracts of 1991 phase 1 projects

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    The objectives of 301 projects placed under contract by the Small Business Innovation Research (SBIR) program of the National Aeronautics and Space Administration (NASA) are described. These projects were selected competitively from among proposals submitted to NASA in response to the 1991 SBIR Program Solicitation. The basic document consists of edited, non-proprietary abstracts of the winning proposals submitted by small businesses. The abstracts are presented under the 15 technical topics within which Phase 1 proposals were solicited. Each project was assigned a sequential identifying number from 001 to 301, in order of its appearance in the body of the report. Appendixes to provide additional information about the SBIR program and permit cross-reference of the 1991 Phase 1 projects by company name, location by state, principal investigator, NASA Field Center responsible for management of each project, and NASA contract number are included

    CMB-S4 Science Book, First Edition

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    This book lays out the scientific goals to be addressed by the next-generation ground-based cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated telescopes at the South Pole, the high Chilean Atacama plateau and possibly a northern hemisphere site, all equipped with new superconducting cameras. CMB-S4 will dramatically advance cosmological studies by crossing critical thresholds in the search for the B-mode polarization signature of primordial gravitational waves, in the determination of the number and masses of the neutrinos, in the search for evidence of new light relics, in constraining the nature of dark energy, and in testing general relativity on large scales

    Ultrasound cleaning of microfilters

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    Report by the ESA-ESO Working Group on Fundamental Cosmology

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    ESO and ESA agreed to establish a number of Working Groups to explore possible synergies between these two major European astronomical institutions. This Working Group's mandate was to concentrate on fundamental questions in cosmology, and the scope for tackling these in Europe over the next ~15 years. One major resulting recommendation concerns the provision of new generations of imaging survey, where the image quality and near-IR sensitivity that can be attained only in space are naturally matched by ground-based imaging and spectroscopy to yield massive datasets with well-understood photometric redshifts (photo-z's). Such information is essential for a range of new cosmological tests using gravitational lensing, large-scale structure, clusters of galaxies, and supernovae. Great scope in future cosmology also exists for ELT studies of the intergalactic medium and space-based studies of the CMB and gravitational waves; here the synergy is less direct, but these areas will remain of the highest mutual interest to the agencies. All these recommended facilities will produce vast datasets of general applicability, which will have a tremendous impact on broad areas of astronomy.Comment: ESA-ESO Working Groups Report No. 3, 125 pages, 28 figures. A PDF version including the cover is available from http://www.stecf.org/coordination/esa_eso/cosmology/report_cover.pdf and a printed version (A5 booklet) is available in limited numbers from the Space Telescope-European Coordinating Facility (ST-ECF): [email protected]

    Trajectory optimization for noise abatement arrival procedures. Case study at Barcelona airport.

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    The main objective of the presented bachelor thesis is the implementation of a trajectory optimizer, based on the minimization of a specific objective function, which describes the noise impact over a set of noise sensitive areas. In order to successfully achieve the desired goal, a convenient noise model is defined where the perceived noise levels are computed as a function of the aircraft trajectory (altitude, speed, thrust, etc.). In addition, the current in-house trajectory optimizer developed by UPC researchers, which before this work only allowed the optimization of the vertical profile (altitude and speed) given a fixed lateral route, has been improved to allow the optimization in the lateral domain by modifying the model describing the aircraft dynamics. Furthermore, with the purpose of obtaining feasible solutions fulfilling the requirements imposed by current air traffic management systems, a set of operational constraints are accurately imposed. Thus, the optimization problem is formulated as an optimal control problem, which is also converted into a non-linear programming problem by means of direct collocation methods. As main contribution of this work, splines interpolation functions are tested with the aim of modeling the measurement grid defining the noise sensitive areas. By doing this, a new unconventional approach is exposed with the intention of proposing an alternative methodology distinct from well-established methods based in implementing discrete points grids, offering then, a simpler way of measuring the noise impact, continuously, through the whole aircraft trajectory. Finally, with the aim of testing the performance of the optimizer, two cases are presented for which different descent trajectories are optimized from the cruise level to the interception of the instrument landing system at three different altitudes (1000, 2000 and 3000 ft). All the results are conveniently exposed with the purpose of obtaining relevant strong evidence-based conclusions. Furthermore, noise footprints are computed with the objective of providing a better visualization of the results. As the results show, the implemented methodology, where splines define the different noise sensitive areas as a continuous, differentiable function, has proven to be more than an effective method, giving very promising results on the two cases exposed

    Science Mission Directorate TechPort Records for 2019 STI-DAA Release

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    The role of the Science Mission Directorate (SMD) is to enable NASA to achieve its science goals in the context of the Nation's science agenda. SMD's strategic decisions regarding future missions and scientific pursuits are guided by Agency goals, input from the science community including the recommendations set forth in the National Research Council (NRC) decadal surveys and a commitment to preserve a balanced program across the major science disciplines. Toward this end, each of the four SMD science divisions -- Heliophysics, Earth Science, Planetary Science, and Astrophysics -- develops fundamental science questions upon which to base future research and mission programs
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