Plant layout analysis and redesign

Includes bibliographical references.SPX is hydraulic company located in Rockford, Illinois that manufactures high-pressure hydraulic components. They make a variety of products that include handpumps, hydraulic pumps to be used in heavy machinery, hydraulic rams and pistons for leveling structures, railroad equipment, cable tools and much more. Our focus for this project is to produce a plan for redesigning the current production floor layout for SPX. To do this we obtained all of the current data for the facility including high-volume part numbers and their routings. After we gained this information we conducted a CORELAP algorithm analysis to determine placement of the departments in the layout. These results were then used to find the optimal layout for the facility and then reanalyze the material flow. Upon comparing the original and revised flow, it was shown that if out improvements were implemented, SPX would save about 15% on material handling costs each year which translates into about $500,000 a year. We recommend implementation of the revised layout due to the fact that the return on investment will only take about a year and overall profits will be significantly higher for SPX in the future.B.S. (Bachelor of Science

Solar Flare X-ray Source Motion as a Response to Electron Spectral Hardening

Context: Solar flare hard X-rays (HXRs) are thought to be produced by nonthermal coronal electrons stopping in the chromosphere, or remaining trapped in the corona. The collisional thick target model (CTTM) predicts that sources produced by harder power-law injection spectra should appear further down the legs or footpoints of a flare loop. Therefore, hardening of the injected power-law electron spectrum during flare onset should be concurrent with a descending hard X-ray source. Aims: To test this implication of the CTTM by comparing its predicted HXR source locations with those derived from observations of a solar flare which exhibits a nonthermally-dominated spectrum before the peak in HXRs, known as an early impulsive event. Methods: HXR images and spectra of an early impulsive C-class flare were obtained using the Ramaty High-Energy Solar Spectroscopic Imager (RHESSI). Images were reconstructed to produce HXR source height evolutions for three energy bands. Spatially-integrated spectral analysis was performed to isolate nonthermal emission, and to determine the power-law index of the electron injection spectrum. The observed height-time evolutions were then fit with CTTM-based simulated heights for each energy. Results: A good match between model and observed source heights was reached, requiring a density model that agreed well with previous studies of flare loop densities. Conclusions: The CTTM has been used to produce a descent of model HXR source heights that compares well with observations of this event. Based on this interpretation, downward motion of nonthermal sources should indeed occur in any flare where there is spectral hardening in the electron distribution during a flare. However, this would often be masked by thermal emission associated with flare plasma pre-heating.Comment: 8 pages, 5 figure

Solar Flare Impulsive Phase Emission Observed with SDO/EVE

Differential emission measures (DEMs) during the impulsive phase of solar flares were constructed using observations from the EUV Variability Experiment (EVE) and the Markov-Chain Monte Carlo method. Emission lines from ions formed over the temperature range log T = 5.8 - 7.2 allow the evolution of the DEM to be studied over a wide temperature range at 10s cadence. The technique was applied to several M- and X-class flares, where impulsive phase EUV emission is observable in the disk-integrated EVE spectra from emission lines formed up to 3 - 4 MK, and we use spatially-unresolved EVE observations to infer the thermal structure of the emitting region. For the nine events studied the DEMs exhibited a two component distribution during the impulsive phase, a low temperature component with peak temperature of 1 - 2 MK, and a broad high temperature one from 7 - 30 MK. A bimodal high temperature component is also found for several events, with peaks at 8 and 25 MK during the impulsive phase. The origin of the emission was verified using AIA images to be the flare ribbons and footpoints, indicating that the constructed DEMs represent the spatially-average thermal structure of the chromospheric flare emission during the impulsive phase.Comment: 18 pages, 6 figures, accepted for publication in Ap

An assessment of Fe XX - Fe XXII emission lines in SDO/EVE data as diagnostics for high density solar flare plasmas using EUVE stellar observations

The Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory obtains extreme-ultraviolet (EUV) spectra of the full-disk Sun at a spectral resolution of ~1 A and cadence of 10 s. Such a spectral resolution would normally be considered to be too low for the reliable determination of electron density (N_e) sensitive emission line intensity ratios, due to blending. However, previous work has shown that a limited number of Fe XXI features in the 90-60 A wavelength region of EVE do provide useful N_e-diagnostics at relatively low flare densities (N_e ~ 10^11-10^12 cm^-3). Here we investigate if additional highly ionised Fe line ratios in the EVE 90-160 A range may be reliably employed as N_e-diagnostics. In particular, the potential for such diagnostics to provide density estimates for high N_e (~10^13 cm^-3) flare plasmas is assessed. Our study employs EVE spectra for X-class flares, combined with observations of highly active late-type stars from the Extreme Ultraviolet Explorer (EUVE) satellite plus experimental data for well-diagnosed tokamak plasmas, both of which are similar in wavelength coverage and spectral resolution to those from EVE. Several ratios are identified in EVE data which yield consistent values of electron density, including Fe XX 113.35/121.85 and Fe XXII 114.41/135.79, with confidence in their reliability as N_e-diagnostics provided by the EUVE and tokamak results. These ratios also allow the determination of density in solar flare plasmas up to values of ~10^13 cm^-3.Comment: 7 pages, 3 figures, 2 tables, MNRAS in pres

Experiences of generating COTS components when automating medicinal product evaluations

This paper reports on experiences of generating COTS components when designing and deploying component based software architecture for automation and interoperation of medicinal product evaluations across different countries in the world. Our generic architectural model renders two sets of software components that are candidates for COTS components. We identify which role such COTS components may play and outline our approach of generating them. We advocate that such COTS components are developed with a specific component platform in mind and must adhere to constraints of our software architecture

Design patterns for automation of marketing authorisations in pharmaceutical industry

This paper reports on the experiences of using existing and creating new design patterns when deploying layered and component based software architecture that automates procedures for marketing authorization. We use the strategy pattern within the generic architecture and deploy the architectural components with the Model-View-Controller (MVC) and front controller patterns. Three domain specific patterns have been created and named as: look-up, submission and evaluation. We advocate that our combination of general and domain specific patterns (i) facilitate the design of distributed software applications, (ii) can be reused in any problem domain where workflows similar to submission and evaluations of application licenses occur, and (iii) comprise commercial-off-the-shelf (COTS) components that fit within our software architecture