Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector

In the low Earth orbit (LEO) neutron particles exist from secondary radiations due to interactions of Galactic Cosmic Ray (GCR) or trapped protons in the Earth's inner radiation belt with the Earth's atmosphere or space object materials or the astronaut themselves. Apart from that, high en...

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Main Authors: Bajuri, F., Bradley, D. A., Mustafa, S., Tamchek, N., Ahmad Saad, F. F., Mazlan, N., Mohd Noor, N.
Format: Article
Published: Elsevier 2022
Online Access:http://psasir.upm.edu.my/id/eprint/102245/
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author Bajuri, F.
Bradley, D. A.
Mustafa, S.
Tamchek, N.
Ahmad Saad, F. F.
Mazlan, N.
Mohd Noor, N.
author_facet Bajuri, F.
Bradley, D. A.
Mustafa, S.
Tamchek, N.
Ahmad Saad, F. F.
Mazlan, N.
Mohd Noor, N.
author_sort Bajuri, F.
building UPM Institutional Repository
collection Online Access
description In the low Earth orbit (LEO) neutron particles exist from secondary radiations due to interactions of Galactic Cosmic Ray (GCR) or trapped protons in the Earth's inner radiation belt with the Earth's atmosphere or space object materials or the astronaut themselves. Apart from that, high energy neutrons produced during solar activities may survive in the distance travelled to the Earth. For passive dosimetry in space, the presence of neutrons should be considered. In this work, we focused on the capability of Customised Optical Fibres (CusOF) to detect the neutrons produced by 241AmBe neutron source. Also, the morphology of flat fibres (FF) was analysed using scanning electron microscopy (SEM) and Electron Dispersive X-ray (EDX). From the SEM images, ImageJ software was employed to measure the area of the organic shaped core of the FF accurately. From the EDX results, it was found that the effective atomic number of CusOF were in the range of 13.40–15.25, similar to human skeleton. Irradiation of CusOF to 241AmBe neutron source shows that at a distance of 0 cm and 15 cm from the source, CusOF had high coefficient of determination (R2) value of 0.95–0.99, better than that of TLD-100 and TLD-700, 0.86 and 0.92, respectively, at 0 cm. This shows that the CusOF has high potential to be used for neutron radiation detector.
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institution Universiti Putra Malaysia
institution_category Local University
last_indexed 2025-11-15T13:37:55Z
publishDate 2022
publisher Elsevier
recordtype eprints
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spelling upm-1022452023-07-10T01:37:35Z http://psasir.upm.edu.my/id/eprint/102245/ Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector Bajuri, F. Bradley, D. A. Mustafa, S. Tamchek, N. Ahmad Saad, F. F. Mazlan, N. Mohd Noor, N. In the low Earth orbit (LEO) neutron particles exist from secondary radiations due to interactions of Galactic Cosmic Ray (GCR) or trapped protons in the Earth's inner radiation belt with the Earth's atmosphere or space object materials or the astronaut themselves. Apart from that, high energy neutrons produced during solar activities may survive in the distance travelled to the Earth. For passive dosimetry in space, the presence of neutrons should be considered. In this work, we focused on the capability of Customised Optical Fibres (CusOF) to detect the neutrons produced by 241AmBe neutron source. Also, the morphology of flat fibres (FF) was analysed using scanning electron microscopy (SEM) and Electron Dispersive X-ray (EDX). From the SEM images, ImageJ software was employed to measure the area of the organic shaped core of the FF accurately. From the EDX results, it was found that the effective atomic number of CusOF were in the range of 13.40–15.25, similar to human skeleton. Irradiation of CusOF to 241AmBe neutron source shows that at a distance of 0 cm and 15 cm from the source, CusOF had high coefficient of determination (R2) value of 0.95–0.99, better than that of TLD-100 and TLD-700, 0.86 and 0.92, respectively, at 0 cm. This shows that the CusOF has high potential to be used for neutron radiation detector. Elsevier 2022 Article PeerReviewed Bajuri, F. and Bradley, D. A. and Mustafa, S. and Tamchek, N. and Ahmad Saad, F. F. and Mazlan, N. and Mohd Noor, N. (2022) Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector. Radiation Physics and Chemistry, 200. pp. 1-12. ISSN 0969-806X; ESSN: 1879-0895 https://www.sciencedirect.com/science/article/pii/S0969806X22004212 10.1016/j.radphyschem.2022.110378
spellingShingle Bajuri, F.
Bradley, D. A.
Mustafa, S.
Tamchek, N.
Ahmad Saad, F. F.
Mazlan, N.
Mohd Noor, N.
Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector
title Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector
title_full Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector
title_fullStr Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector
title_full_unstemmed Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector
title_short Morphology and thermoluminescence characteristics of customised Ge-doped optical fibre under Am-Be neutron source as a potential to be used for space radiation detector
title_sort morphology and thermoluminescence characteristics of customised ge-doped optical fibre under am-be neutron source as a potential to be used for space radiation detector
url http://psasir.upm.edu.my/id/eprint/102245/
http://psasir.upm.edu.my/id/eprint/102245/
http://psasir.upm.edu.my/id/eprint/102245/