371 research outputs found

    Virtual Reality and its Applications in the Mockup Process: A Case Study

    Get PDF
    Mockups are an important part of the construction process as they provide numerous benefits in both constructability review and aesthetic approval. Virtual Reality is an emerging technology that could prove to be a valuable addition to the mockup process. Many construction firms are attempting to incorporate virtual reality into any process they can --ranging from impressing owners in order to procure jobs to training employees so they can more adeptly adjust to field conditions. This paper will introduce virtual reality and some of its applications in the construction industry, specifically analyzing virtual reality and its applications in the mockup process via a case study. While the projects were met largely with success, they had their share of challenges in implementation. VR mockups proved valuable for aesthetic review purposes. They also improved the design-approval process which, in turn, reduced both cost and time. The technology was still met with challenges in implementation. The primary challenges were: aversion to the new technology, illness/nausea, hesitation about increased investment earlier in the project, and the reliance on available technology

    ASTR 131.01: Elementary Astronomy I

    Get PDF

    ASTR 363.01: Stellar Astronomy and Astrophysics I

    Get PDF

    SCI 225.01: General and Chemical Science

    Get PDF

    ASTR 351.01: Planetary Science

    Get PDF

    GEOL 351.01: Planetary Science

    Get PDF

    Implementation of a Rapid Assessment Unit (Intake Team): Impact on Emergency Department Length of Stay

    Get PDF
    Implementation of a Rapid Assessment Unit (Intake Team): Impact on Emergency Department Length of Stay Richard S. MacKenzie, MD, David B. Burmeister, DO, Jennifer A. Brown, RN, Melissa Teitsworth, RN, BSN, Christopher J. Kita, MEd, Megan J. Dambach, DO, Shaheen Shamji, DO, Anita Kurt, PhD, RN , Susan Friend, Marna Greenberg, DO, MPH Acknowledge: Clare M. Lenhart, PhD, MPH Objective: Emergency Department (ED) crowding is an on-going formidable issue for many EDs. A Rapid Assessment Unit (RAU) is a potential solution. This process involves the use of a team approach to convert the current “series” type evaluation to a more “parallel” evaluation and treatment of patients. The RAU concept of evaluating and treating ED patients radically changes the current methods utilized in today’s standard emergency care area. The RAU concept offers a process in which the patient walks into the ED and is seen in a unit by an intake team composed of a nurse, registrar, and provider (physician assistant, nurse practitioner, or physician) that provides evaluation and emergent treatment. This removes the redundancy of a patient giving the same information several times before they are treated. Simultaneously, the team decides whether the patient would be better served by remaining seated or requires a recumbent position. This is referred to as allowing “vertical flow” versus the default “horizontal flow” where all patients recline on a stretcher whether they need it or not. Certainly, having construction that specifically supports these processes is an innovation as well (having an area where patients can be seated and remain “vertical”). The team structure itself is unique. The nurses and providers are not assigned geographically by room but rather are defined by their function. We set out to determine if the addition of the RAU process would decreases the LOS of the discharged ambulatory arrival patient. Methods: After IRB approval, this retrospective, pre- and post intervention, observational comparison study was conducted from August 2011-March 2012 at a suburban teaching hospital in central Pennsylvania with an annual ED census of approximately 54,000. The inclusion criteria were all ambulatory discharged patients. The exclusion criteria were all patients that arrived by ambulance and admitted patients. Data points captured included: time of arrival in triage , time in triage to ED entry, time of ED entry until seen by a provider, time from ED entry to discharge, total length of stay (LOS). The data were uploaded to Horizon Business Insightℱ (HBI), a cumulative data manager and exported to an Microsoft excel file for analysis. Mann-Whitney U tests were used to demonstrate differences in Median LOS. All statistical tests were 2-sided; probability values \u3c0.05 were considered significant. Results: 11, 994 pre and 10814 post-RAU patients were included in analysis. Median LOS was shorter during the post-RAU period in each subcategory of LOS with the exception of the interval from being seen in the ER to discharge which is a result of provider seeing the patient earlier in the ED encounter. Results, Table 1. Conclusions: The RAU process decreases the LOS of the discharged ambulatory arrival patient and deserves further exploration as an innovative model in the ED that improves flow

    J-band spectroscopy of cataclysmic variables

    Get PDF
    We present time-resolved, J-band (1.025–1.340 ÎŒm) infrared spectra of the short-period dwarf novae (DNe) WZ Sge and VY Aqr, and single spectra of the short-period DN EF Peg and the nova-like variable PX And. There is some evidence in the spectra of VY Aqr and EF Peg that we have detected the secondary star, both in the continuum slope and also through the possible presence of spectral features. The spectra of WZ Sge and PX And, on the other hand, show no evidence for the secondary star, with upper limits for its contribution to the J-band light of 10 and 20 per cent respectively. The spectral type of the secondary in WZ Sge is constrained to be later than M7.5V. Using skew mapping, we have been able to derive a value for the radial velocity semi-amplitude of the secondary star in VY Aqr of KR=320±70 km s−1, which in conjunction with KW from Thorstensen & Taylor gives a mass ratio of q=0.15±0.04

    Superhumps in Cataclysmic Binaries. XXIV. Twenty More Dwarf Novae

    Full text link
    We report precise measures of the orbital and superhump period in twenty more dwarf novae. For ten stars, we report new and confirmed spectroscopic periods - signifying the orbital period P_o - as well as the superhump period P_sh. These are GX Cas, HO Del, HS Vir, BC UMa, RZ Leo, KV Dra, KS UMa, TU Crt, QW Ser, and RZ Sge. For the remaining ten, we report a medley of P_o and P_sh measurements from photometry; most are new, with some confirmations of previous values. These are KV And, LL And, WX Cet, MM Hya, AO Oct, V2051 Oph, NY Ser, KK Tel, HV Vir, and RX J1155.4-5641. Periods, as usual, can be measured to high accuracy, and these are of special interest since they carry dynamical information about the binary. We still have not quite learned how to read the music, but a few things are clear. The fractional superhump excess epsilon [=(P_sh-P_o)/P_o] varies smoothly with P_o. The scatter of the points about that smooth curve is quite low, and can be used to limit the intrinsic scatter in M_1, the white dwarf mass, and the mass-radius relation of the secondary. The dispersion in M_1 does not exceed 24%, and the secondary-star radii scatter by no more than 11% from a fixed mass-radius relation. For the well-behaved part of epsilon(P_o) space, we estimate from superhump theory that the secondaries are 18+-6% larger than theoretical ZAMS stars. This affects some other testable predictions about the secondaries: at a fixed P_o, it suggests that the secondaries are (compared with ZAMS predictions) 40+-14% less massive, 12+-4% smaller, 19+-6% cooler, and less luminous by a factor 2.5(7). The presence of a well-defined mass-radius relation, reflected in a well-defined epsilon(P_o) relation, strongly limits effects of nuclear evolution in the secondaries.Comment: PDF, 62 pages, 7 tables, 21 figures; accepted, in press, to appear November 2003, PASP; more info at http://cba.phys.columbia.edu

    Singlet exciton fission in solution.

    Get PDF
    Singlet exciton fission, the spin-conserving process that produces two triplet excited states from one photoexcited singlet state, is a means to circumvent the Shockley-Queisser limit in single-junction solar cells. Although the process through which singlet fission occurs is not well characterized, some local order is thought to be necessary for intermolecular coupling. Here, we report a triplet yield of 200% and triplet formation rates approaching the diffusion limit in solutions of bis(triisopropylsilylethynyl (TIPS)) pentacene. We observe a transient bound excimer intermediate, formed by the collision of one photoexcited and one ground-state TIPS-pentacene molecule. The intermediate breaks up when the two triplets separate to each TIPS-pentacene molecule. This efficient system is a model for future singlet-fission materials and for disordered device components that produce cascades of excited states from sunlight.B.J.W. was supported by a Herchel Smith Research Fellowship. A.J.M. received funding from a Marie Curie Scholarship. D.B. is a FNRS Research Director. Both A.J.M and D.B. acknowledge support from the European Community’s Initial Training Network SUPERIOR (PITN-GA-2009-238177). Further funding for this project came from the Engineering and Physical Sciences Research Council (EPSRC) and a pump-prime grant from the Winton Programme for the Physics of Sustainability.This is the accepted version of an article originally published in Nature Chemistry 5, 1019–1024 and available online at http://www.nature.com/nchem/journal/v5/n12/full/nchem.1801.html. Nature Publishing Group's conditions for reuse are detailed at http://www.nature.com/authors/policies/license.html
    • 

    corecore