The Secondary Scintillation of Rare Gases under the Influence of Magnetic Fields
Autor(a) principal: | |
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Data de Publicação: | 1980 |
Outros Autores: | , , |
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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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 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.publisher.none.fl_str_mv |
IEEE |
publisher.none.fl_str_mv |
IEEE |
dc.source.none.fl_str_mv |
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Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
instacron_str |
RCAAP |
institution |
RCAAP |
reponame_str |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
collection |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
repository.name.fl_str_mv |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
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1799133889444184064 |