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The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps

Dissertation (MSc)--University of Pretoria, 2019.

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Other Authors: Meyer, W.E. (Walter Ernst)
Format: Thesis
Language:English
Published: University of Pretoria 2019
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access_status_str Open Access
author2 Meyer, W.E. (Walter Ernst)
author_browse Meyer, W.E. (Walter Ernst)
author_facet Meyer, W.E. (Walter Ernst)
collection Thesis
dc_rights_str_mv © 2019 University of Pretoria. All rights reserved. The copyright in this work vests in the University of Pretoria. No part of this work may be reproduced or transmitted in any form or by any means, without the prior written permission of the University of Pretoria.
description Dissertation (MSc)--University of Pretoria, 2019.
format Thesis
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institution University of Pretoria (South Africa)
language English
last_indexed 2026-06-10T12:39:34.803Z
license_str Other — see source repository
provenance_str_mv Harvested via OAI-PMH from UPSpace — University of Pretoria Institutional Repository
publishDate 2019
publishDateRange 2019
publishDateSort 2019
publisher University of Pretoria
publisherStr University of Pretoria
record_format dspace
source_str UPSpace — University of Pretoria Institutional Repository
spelling oai:repository.up.ac.za:2263/68544 The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps Meyer, W.E. (Walter Ernst) ketani.elliot@gmail.com Du Toit, Pieter Johannes Wynand Sieberhagen, Rheinhardt Hendrik Mkabela, Macdufe UCTD Physics Dissertation (MSc)--University of Pretoria, 2019. The measurement of spectral irradiance in the ultraviolet (UV) region of the electromagnetic spectrum has higher uncertainties largely due to a low signal-to-noise ratio (SNR). UV-C radiation emitted by low pressure (LP) mercury (Hg) lamps is very important in a wide range of applications including disinfection of air and surfaces of microorganisms. This study investigates some measurement aspects to be considered when calibrating LP Hg lamps. The aim is to characterise the spectroradiometer system and improve measurement techniques for calibrating this lamp for use as a source standard for disseminating the unit of spectral irradiance in the UV-C spectral region. The research question is answered through an experiment that includes a direct measurement of a LP Hg lamp against a deuterium (D2) standard (STD) lamp. The measurements showed that the alignment of the LP Hg lamp should be a primary concern as this aspect contributed 15 % to the combined uncertainty. Ambient temperature changes are known to influence some components used in the measurement of spectral irradiance. In this regard, the study indicated that the LP Hg lamp may be operated at lower temperatures to achieve maximum light output. The lamp has a calculated temperature coefficient of -2,5 \pm 0,01 % oC at an ambient temperature of 21,3 oC. During measurements, a short-term drift of a measurand can be an obstacle to lamp spectral irradiance calibration. The cause is frequently heat build-up and temperature changes in the components of a spectroradiometer. The spectroradiometer had a higher measured short-term drift of 5 % when irradiated with a LP Hg lamp compared to 1 % when irradiated with a D2 STD lamp. Apart from a higher measured drift, the lamp’s light output was more stable over time when monitored with UV enhanced silicon (Si) detectors: 1,6 % for a LP Hg lamp and 0,11 % for a D2 STD lamp. The LP Hg lamp had a calibrated total UV irradiance of 1,12 W/m2 from 230 nm to 400 nm wavelengths. The expanded uncertainty was 8 % which is lower than 11 % uncertainty that the National Metrology Institute of South Africa (NMISA) is accredited for. This showed that even though the spectroradiometer system had a higher measured short-term drift when irradiated with a LP Hg lamp, the lamps can be used as a source standard for calibrating clients’ instruments. Further research must be conducted to identify and characterise other measurement aspects that could have significant uncertainty contributions. Physics MSc Unrestricted 2019-03-04T08:27:55Z 2019-03-04T08:27:55Z 2019-04-11 2019 Dissertation Mkabela, M 2019, The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps, MSc Dissertation, University of Pretoria, Pretoria, viewed yymmdd <http://hdl.handle.net/2263/68544> A2019 http://hdl.handle.net/2263/68544 en © 2019 University of Pretoria. All rights reserved. The copyright in this work vests in the University of Pretoria. No part of this work may be reproduced or transmitted in any form or by any means, without the prior written permission of the University of Pretoria. application/pdf University of Pretoria
spellingShingle UCTD
Physics
The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps
title The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps
title_full The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps
title_fullStr The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps
title_full_unstemmed The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps
title_short The development of a measuring technique for the UV-C distribution emitted from low pressure mercury lamps
title_sort development of a measuring technique for the uv c distribution emitted from low pressure mercury lamps
topic UCTD
Physics
url http://hdl.handle.net/2263/68544