Procedure for verification of sound source coverage over façades according to the International Standard ISO 140-5

This paper presents a new verification procedure for sound source coverage according to ISO 140?5 requirements. The ISO 140?5 standard applies to the measurement of façade insulation and requires a sound source able to achieve a sufficiently uniform sound field in free field conditions on the façade under study. The proposed method involves the electroacoustic characterisation of the sound source in laboratory free field conditions (anechoic room) and the subsequent prediction by computer simulation of the sound free field radiated on a rectangular surface equal in size to the façade being measured. The loudspeaker is characterised in an anechoic room under laboratory controlled conditions, carefully measuring directivity, and then a computer model is designed to calculate the acoustic free field coverage for different loudspeaker positions and façade sizes. For each sound source position, the method provides the maximum direct acoustic level differences on a façade specimen and therefore determines whether the loudspeaker verifies the maximum allowed level difference of 5 dB (or 10 dB for façade dimensions greater than 5 m) required by the ISO standard. Additionally, the maximum horizontal dimension of the façade meeting the standard is calculated and provided for each sound source position, both with the 5 dB and 10 dB criteria. In the last section of the paper, the proposed procedure is compared with another method used by the authors in the past to achieve the same purpose: in situ outdoor measurements attempting to recreate free field conditions. From this comparison, it is concluded that the proposed method is able to reproduce the actual measurements with high accuracy, for example, the ground reflection effect, at least at low frequencies, which is difficult to avoid in the outdoor measurement method, and it is fully eliminated with the proposed method to achieve the free field requisite.

Caracterización del Acabado Superficial en la Industria Aeronautica y Aeroespacial - Desarrollo de Software Patrón de Referencia de Acuerdo a la Norma ISO 5436: VisualSR2D

This BSc thesis introduces the development of an independent, standalone software, VisualSR2D, for the characterization of software roughness. The software is written in Matlab, can be installed in any Windows OS as an standalone application and is available under request. It is intended to be an alternative for Softgauges (National Physical Laboratory, UK), RPTB (Physikalisch-Technische Bundesanstal, Germany) and SMATS (National Institute of Standards and Technology, USA) in the study of surface roughness. The standard ISO 5436-2 is presented, the above mentioned alternative developments are analyzed and compared, best practices are gathered, and finally, the development and functionality of VisualSR2D is presented.

Proposta e avaliação de uma sistemática para a implementação da norma ISO 22000: 2005 - sistemas de gestão da segurança de alimentos e exemplo prático de sua implementação

Foi desenvolvida uma proposta de sistemática para implementação de Sistema de Gestão da Segurança de Alimentos com base na Norma ISO 22000:2005 (NBR ISO 22000:2006). Esta sistemática está composta por: A) Mapeamento da documentação; B) Formulários para o Planejamento do sistema APPCC/ HACCP com base na norma ISO 22000, bem como Instrução para seu uso, incluindo tanto as etapas preliminares como os 7 Princípios estabelecidos pelo Codex Alimentarius; C) Documentos para a verificação dos sistemas: Checklist para auditoria de verificação, tanto de adequação como de implementação, e Mapeamento da comunicação. Esta sistemática foi aplicada em uma linha de produtos em pó de empresa real, de porte médio, denominada, ficticiamente, empresa EXEMPLO. Foram dados os treinamentos necessários, adequados ao nível de conhecimento da equipe de segurança de alimentos, e realizadas reuniões de consultoria. Após implementação da sistemática proposta pela equipe da empresa EXEMPLO na linha de produtos escolhida para este fim, foi realizada uma auditoria de verificação para a avaliação da adequação do Sistema de Gestão da Segurança de Alimentos com base na Norma ISO 22000. A equipe foi composta por três auditores, sendo dois deles com formação nível auditor líder de ISO 22000. Concluiu-se que a sistemática é eficaz e adequada, atendendo plenamente às exigências da Norma ISO 22000. Foi, também, incluído no trabalho exemplo prático da documentação básica resultante da implementação na empresa EXEMPLO. A sistemática e modelos desenvolvidos, bem como a visualização de um exemplo prático, podem auxiliar as empresas a diminuir significativamente o tempo de implementação, embora ajustes devam ser feitos para adequação à sua realidade. Os ajustes necessários devem considerar os requisitos regulamentares, dependendo do tipo de produto e do órgão regulatório responsável pela sua regulamentação e fiscalização, bem como requisitos estatutários que possam impactar na sistemática desenvolvida.

The circumstellar environment and evolutionary status of the supergiant B[e] star Wd1-9

Context. Historically, supergiant (sg)B[e] stars have been difficult to include in theoretical schemes for the evolution of massive OB stars. Aims. The location of Wd1-9 within the coeval starburst cluster Westerlund 1 means that it may be placed into a proper evolutionary context and we therefore aim to utilise a comprehensive multiwavelength dataset to determine its physical properties and consequently its relation to other sgB[e] stars and the global population of massive evolved stars within Wd1. Methods. Multi-epoch R- and I-band VLT/UVES and VLT/FORS2 spectra are used to constrain the properties of the circumstellar gas, while an ISO-SWS spectrum covering 2.45−45μm is used to investigate the distribution, geometry and composition of the dust via a semi-analytic irradiated disk model. Radio emission enables a long term mass-loss history to be determined, while X-ray observations reveal the physical nature of high energy processes within the system. Results. Wd1-9 exhibits the rich optical emission line spectrum that is characteristic of sgB[e] stars. Likewise its mid-IR spectrum resembles those of the LMC sgB[e] stars R66 and 126, revealing the presence of equatorially concentrated silicate dust, with a mass of ~10−4M⊙. Extreme historical and ongoing mass loss (≳ 10−4M⊙yr−1) is inferred from the radio observations. The X-ray properties of Wd1-9 imply the presence of high temperature plasma within the system and are directly comparable to a number of confirmed short-period colliding wind binaries within Wd1. Conclusions. The most complete explanation for the observational properties of Wd1-9 is that it is a massive interacting binary currently undergoing, or recently exited from, rapid Roche-lobe overflow, supporting the hypothesis that binarity mediates the formation of (a subset of) sgB[e] stars. The mass loss rate of Wd1-9 is consistent with such an assertion, while viable progenitor and descendent systems are present within Wd1 and comparable sgB[e] binaries have been identified in the Galaxy. Moreover, the rarity of sgB[e] stars - only two examples are identified from a census of ~ 68 young massive Galactic clusters and associations containing ~ 600 post-Main Sequence stars - is explicable given the rapidity (~ 104yr) expected for this phase of massive binary evolution.

Oil Retention and Pressure Drop in Horizontal and Vertical Suction Lines with R410A / POE ISO 32

In refrigeration systems a small amount of compressor lubricant is entrained in the refrigerant and circulated through the system, where some is retained in each component. The suction line to the compressor has the largest potential for oil retention. This paper presents results from an experimental apparatus that has been constructed to circulate POE (polyolester) oil and R410A at a controlled mass flux, OCR (oil in circulation ratio), and apparent superheat, and to directly measure the pressure drop and mass of oil retained in horizontal and vertical suction lines. The bulk vapor velocity and overall void fraction are determined from direct mass and temperature measurements. The oil retention, pressure drop, and flow regimes near the minimum ASHRAE recommended mass flux condition are explored. It was found that oil retention begins to increase sharply even above the minimum recommended flux, so conditions near the minimum should be avoided. Two relationships were developed to predict the oil retention in the vertical and horizontal suction lines. The average error from the predictions method was 10.9% for the vertical tube, and 7.9% for the horizontal tube.