The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields

Detalhes bibliográficos
Autor(a) principal: Ferreira, M. Fátima A.
Data de Publicação: 1980
Outros Autores: Conde, C. A. N., Campos, N. Ayres de, Gil, J. M. S. C.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10316/12900
https://doi.org/10.1109/TNS.1980.4330829
Resumo: The influence of magnetic fields on the secondary scintillation of xenon and argon is studied. A small gas cell is used with excitation by alpha-particles and magnetic fields perpendicular to the direction of the electric fields. For reduced electric fields normally used in gas proportional scintillation counters the intensity of the secondary scintillation remains constant, within an accuracy of about ± 1 % for xenon and ± 2% for argon, when the magnetic field intensity varied from 0 to 0.4 Tesla. A discussion and interpretation of the experimental data obtained is presented. It is concluded that gas proportional scintillation counters can be used in high magnetic field environments
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spelling The Secondary Scintillation of Rare Gases under the Influence of Magnetic FieldsThe influence of magnetic fields on the secondary scintillation of xenon and argon is studied. A small gas cell is used with excitation by alpha-particles and magnetic fields perpendicular to the direction of the electric fields. For reduced electric fields normally used in gas proportional scintillation counters the intensity of the secondary scintillation remains constant, within an accuracy of about ± 1 % for xenon and ± 2% for argon, when the magnetic field intensity varied from 0 to 0.4 Tesla. A discussion and interpretation of the experimental data obtained is presented. It is concluded that gas proportional scintillation counters can be used in high magnetic field environmentsIEEE1980-02info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://hdl.handle.net/10316/12900http://hdl.handle.net/10316/12900https://doi.org/10.1109/TNS.1980.4330829engIEEE Transactions on Nuclear Science 27:1 (1980) 208-2110018-9499Ferreira, M. Fátima A.Conde, C. A. N.Campos, N. Ayres deGil, J. M. S. C.info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2020-11-06T17:00:09Zoai:estudogeral.uc.pt:10316/12900Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T20:59:54.929642Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
title The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
spellingShingle The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
Ferreira, M. Fátima A.
title_short The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
title_full The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
title_fullStr The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
title_full_unstemmed The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
title_sort The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
author Ferreira, M. Fátima A.
author_facet Ferreira, M. Fátima A.
Conde, C. A. N.
Campos, N. Ayres de
Gil, J. M. S. C.
author_role author
author2 Conde, C. A. N.
Campos, N. Ayres de
Gil, J. M. S. C.
author2_role author
author
author
dc.contributor.author.fl_str_mv Ferreira, M. Fátima A.
Conde, C. A. N.
Campos, N. Ayres de
Gil, J. M. S. C.
description The influence of magnetic fields on the secondary scintillation of xenon and argon is studied. A small gas cell is used with excitation by alpha-particles and magnetic fields perpendicular to the direction of the electric fields. For reduced electric fields normally used in gas proportional scintillation counters the intensity of the secondary scintillation remains constant, within an accuracy of about ± 1 % for xenon and ± 2% for argon, when the magnetic field intensity varied from 0 to 0.4 Tesla. A discussion and interpretation of the experimental data obtained is presented. It is concluded that gas proportional scintillation counters can be used in high magnetic field environments
publishDate 1980
dc.date.none.fl_str_mv 1980-02
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10316/12900
http://hdl.handle.net/10316/12900
https://doi.org/10.1109/TNS.1980.4330829
url http://hdl.handle.net/10316/12900
https://doi.org/10.1109/TNS.1980.4330829
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv IEEE Transactions on Nuclear Science 27:1 (1980) 208-211
0018-9499
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eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv IEEE
publisher.none.fl_str_mv IEEE
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