7,654 research outputs found

    Improving quality consistency and productivity of color separators utilizing the Dupont image manager

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    The magic key in any commercial transaction is to satisfy the customer\u27s requirements. In the color separation market the customer\u27s expectations are consistency in the product, and films that when printed will reproduce a clean visual match to the original copy. The variables that affect the quality, consistency, and productivity for the color separation process, were reviewed. The result of this review was that the operator\u27s scanner set-up for tone reproduction is the most critical variable in the process. An estimate of the total cost in the United States caused by rescans due to inconsistency of the scanner set-up gave the result of $462,852,000 per year. One solution to the problem of inconsistency of the scanner set-up seems to be the use of pre-scan systems. The pre-scan system helps the scanner operator determinate the optimum tone reproduction for each color separation. A review of the related literature described seven presetter and seven presetter/previewer systems. To test pre-scan effectiveness the DuPont Image Manager was used to produce the suggested scanner set-up using a computerized method for the tone reproduction determination with very little operator assistance. This study answered the research question, does the DuPont Image Manager improve the quality, consistency, and productivity of color separations made on a Hell DC 399 Scanner? The Hell DC 399 scanner was used. Two hypotheses, and the experimental design are presented. The experiment produced color separations using the judgment of three experienced and three inexperienced scanner operators, and by using the pre-scan system. With the films obtained, Cromalin color proofs were made. Judges evaluated the proofs using pair comparison to study the quality consistency improvement. To study the productivity, the average time required for the scanner set-up using both methods was measured, using the scanner operator\u27s judgment and the DuPont Image Manager. The results of the study yielded the following conclusions: the overall visual preference of color separations was higher when the scanner is set-up according to the Du Pont Image Manager instructions by experienced or inexperienced scanner operators. The Du Pont Image Manager produces an improvement in the productivity of setting up a scanner in a ratio of 45% for the inexperienced scanner operators. The use of the Du Pont Image Manager did not significantly increase the color separation acceptance either for experienced or inexperienced scanner operators, or for different kind of originals. For low key originals, the operator\u27s judgment produced a better overall visual color separation, compared to when the Image Manager was used. For high key originals there is no difference in the visual preference for the color separations made using either one of the two methods analyzed. For normal key, over exposed, and under exposed originals the visual preference was higher for those color separations that were made following the Du Pont Image Manager instructions for the scanner set-up. The recommendation for further study is that the same research can be performed in a real working situation, at five or six shops, using their normal jobs in the test, and asking their customers to judge the separation\u27s acceptance

    Aplicación de una red social como herramienta docente en asignaturas tecnológicas

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    Póster presentado en: VIII Jornadas de Innovación Docente de la UBU, Burgos, 5 de abril de 2016, organizadas por el Instituto de Formación e Innovación Educativa-IFIE de la Universidad de Burgo

    The UN in the lab

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    We consider two alternatives to inaction for governments combating terrorism, which we term Defense and Prevention. Defense consists of investing in resources that reduce the impact of an attack, and generates a negative externality to other governments, making their countries a more attractive objective for terrorists. In contrast, Prevention, which consists of investing in resources that reduce the ability of the terrorist organization to mount an attack, creates a positive externality by reducing the overall threat of terrorism for all. This interaction is captured using a simple 3×3 “Nested Prisoner’s Dilemma” game, with a single Nash equilibrium where both countries choose Defense. Due to the structure of this interaction, countries can benefit from coordination of policy choices, and international institutions (such as the UN) can be utilized to facilitate coordination by implementing agreements to share the burden of Prevention. We introduce an institution that implements a burden-sharing policy for Prevention, and investigate experimentally whether subjects coordinate on a cooperative strategy more frequently under different levels of cost sharing. In all treatments, burden sharing leaves the Prisoner’s Dilemma structure and Nash equilibrium of the game unchanged. We compare three levels of burden sharing to a baseline in a between-subjects design, and find that burden sharing generates a non-linear effect on the choice of the efficient Prevention strategy and overall performance. Only an institution supporting a high level of mandatory burden sharing generates a significant improvement in the use of the Prevention strategy

    Controle biológico de percevejos fitófagos da soja na região de Dourados, MS.

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    Este trabalho teve como objetivo avaliar o parasitismo natural que ocorre em adultos e em ovos do percevejo-marrom da soja Euschistus heros (Fabricius), bem como multiplicar o parasitóide Telenomus podisi (Ashmead) e liberá-lo em lavouras de soja, visando ao controle biológico do percevejo nesta cultura. Durante a safra 2004/2005 e 2005/2006 e nas entressafras de 2004, 2005 e 2006 foram coletados adultos do percevejo, enquanto nas safras de 2003/2004 e 2004/2005 foram coletadas massas de ovos do inseto durante o período reprodutivo da sojabitstream/item/38732/1/BP200740.pdfDocumento on-line

    Area selection for conservation of Mexican mammals

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    Three sets of priority cells for mammal conservation in Mexico were identified using distributional data. A complementarity approach was implemented through linear integer programming. The minimum set of sites required for the representation of each mammal species varied between 38 (5.4%) grid cells for at least one occurrence, 110 (15.6%) grid cells for at least three occurrences, and 173 (24.5%) grid cells for at least five occurrences. The complementary analyses mainly highlighted three regions of particular concern for mammal conservation in Mexico: (i) the trans-Mexican Volcanic Belt and natural provinces of the Pacific Coast, (ii) Sierra Madre del Sur and the Highlands of Chiapas, and (iii) the northern portion of the Sierra Madre Occidental. The results reported here did not indicate absolute priority locations for conservation activities, but rather identified locations warranting further investigation at finer resolutions more appropriate to such activit

    Warm SiO gas in molecular bullets associated with protostellar outflows

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    In this paper we present the first SiO multiline analysis (from J=2-1 to J=11-10) of the molecular bullets along the outflows of the Class 0 sources L1448-mm and L1157-mm, obtained through observations with IRAM and JCMT. We have computed the main physical parameters in each bullet and compared them with other tracers of warm and dense gas and with models for the SiO excitation in shocks. We find that the bullets close to L1448--mm, associated with high velocity gas, have higher excitation conditions (n(H2) ~ 10^{6} cm^{-3}, T > 500 K) with respect to the L1157 bullets (n(H2) ~1-5 10^{5} cm^{-3}, T ~ 100-300 K). In both the sources, there is a clear evidence of the presence of velocity components having different excitation conditions, with the denser and/or warmer gas associated with the gas at the higher speed. In L1448 the bulk of the emission is due to the high-excitation and high velocity gas, while in L1157 most of the emission comes from the low excitation gas at ambient velocity. The observed velocity-averaged line ratios are well reproduced by shocks with speeds v_s larger than ~ 30 km/s and densities ~ 10^{5} - 10^{6} cm^{-3}. Plane-parallel shock models, however, fail to predict all the observed line profiles and in particular the very similar profiles shown by both low and high excitation lines. The overall observations support the idea that the L1157 clumps are shock interaction events older than the L1448 bullets close to the driving source. In the latter objects, the velocity structure and the variations of physical parameters with the velocity resemble very closely those found in optical/IR jets near the protostar, suggesting that similar launching and excitation mechanisms are also at the origin of collimated jets seen at millimetre wavelengths.Comment: 11pages, 9 figures, A&A accepte

    Jets and Outflows From Star to Cloud: Observations Confront Theory

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    In this review we focus on the role jets and outflows play in the star and planet formation process. Our essential question can be posed as follows: are jets/outflows merely an epiphenomenon associated with star formation or do they play an important role in mediating the physics of assembling stars both individually and globally? We address this question by reviewing the current state of observations and their key points of contact with theory. Our review of jet/outflow phenomena is organized into three length-scale domains: Source and Disk Scales (0.11020.1-10^2 au) where the connection with protostellar and disk evolution theories is paramount; Envelope Scales (10210510^2-10^5 au) where the chemistry and propagation shed further light on the jet launching process, its variability and its impact on the infalling envelope; Parent Cloud Scales (10510610^5-10^6 au) where global momentum injection into cluster/cloud environments become relevant. Issues of feedback are of particular importance on the smallest scales where planet formation regions in a disk may be impacted by the presence of disk winds, irradiation by jet shocks or shielding by the winds. Feedback on envelope scales may determine the final stellar mass (core-to-star efficiency) and envelope dissipation. Feedback also plays an important role on the larger scales with outflows contributing to turbulent support within clusters including alteration of cluster star formation efficiencies (feedback on larger scales currently appears unlikely). A particularly novel dimension of our review is that we consider results on jet dynamics from the emerging field of High Energy Density Laboratory Astrophysics (HEDLA). HEDLA is now providing direct insights into the 3-D dynamics of fully magnetized, hypersonic, radiative outflows.Comment: Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. Klessen, C. Dullemond, Th. Hennin
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