Nitrogen fluorescence in air for observing extensive air showers

Detalhes bibliográficos
Autor(a) principal: Keilhauer, B.
Data de Publicação: 2012
Outros Autores: Bohacova, M., Fraga, M. M. F. R., Matthews, J., Sakaki, N., Tameda, Y., Tsunesada, Y., Ulrich, A.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10316/109735
https://doi.org/10.1051/epjconf/20135301010
Resumo: 12 pages, 17 figures, 2 tables, International Symposium on Future Directions in UHECR Physics, 13-16 February 2012, CERN, Geneva (Switzerland); the updated version corrects for a typo in Eq. (1)
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spelling Nitrogen fluorescence in air for observing extensive air showersastro-ph.HEastro-ph.IM12 pages, 17 figures, 2 tables, International Symposium on Future Directions in UHECR Physics, 13-16 February 2012, CERN, Geneva (Switzerland); the updated version corrects for a typo in Eq. (1)Extensive air showers initiate the fluorescence emissions from nitrogen molecules in air. The UV-light is emitted isotropically and can be used for observing the longitudinal development of extensive air showers in the atmosphere over tenth of kilometers. This measurement technique is well-established since it is exploited for many decades by several cosmic ray experiments. However, a fundamental aspect of the air shower analyses is the description of the fluorescence emission in dependence on varying atmospheric conditions. Different fluorescence yields affect directly the energy scaling of air shower reconstruction. In order to explore the various details of the nitrogen fluorescence emission in air, a few experimental groups have been performing dedicated measurements over the last decade. Most of the measurements are now finished. These experimental groups have been discussing their techniques and results in a series of Air Fluorescence Workshops commenced in 2002. At the 8$^{\rm{th}}$ Air Fluorescence Workshop 2011, it was suggested to develop a common way of describing the nitrogen fluorescence for application to air shower observations. Here, first analyses for a common treatment of the major dependences of the emission procedure are presented. Aspects like the contributions at different wavelengths, the dependence on pressure as it is decreasing with increasing altitude in the atmosphere, the temperature dependence, in particular that of the collisional cross sections between molecules involved, and the collisional de-excitation by water vapor are discussed.EDP Sciences2012-10-04info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://hdl.handle.net/10316/109735http://hdl.handle.net/10316/109735https://doi.org/10.1051/epjconf/20135301010eng2100-014Xhttp://arxiv.org/abs/1210.1319v2Keilhauer, B.Bohacova, M.Fraga, M. M. F. R.Matthews, J.Sakaki, N.Tameda, Y.Tsunesada, Y.Ulrich, A.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:RCAAP2023-10-24T12:21:41Zoai:estudogeral.uc.pt:10316/109735Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T21:25:53.266952Repositório 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 Nitrogen fluorescence in air for observing extensive air showers
title Nitrogen fluorescence in air for observing extensive air showers
spellingShingle Nitrogen fluorescence in air for observing extensive air showers
Keilhauer, B.
astro-ph.HE
astro-ph.IM
title_short Nitrogen fluorescence in air for observing extensive air showers
title_full Nitrogen fluorescence in air for observing extensive air showers
title_fullStr Nitrogen fluorescence in air for observing extensive air showers
title_full_unstemmed Nitrogen fluorescence in air for observing extensive air showers
title_sort Nitrogen fluorescence in air for observing extensive air showers
author Keilhauer, B.
author_facet Keilhauer, B.
Bohacova, M.
Fraga, M. M. F. R.
Matthews, J.
Sakaki, N.
Tameda, Y.
Tsunesada, Y.
Ulrich, A.
author_role author
author2 Bohacova, M.
Fraga, M. M. F. R.
Matthews, J.
Sakaki, N.
Tameda, Y.
Tsunesada, Y.
Ulrich, A.
author2_role author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Keilhauer, B.
Bohacova, M.
Fraga, M. M. F. R.
Matthews, J.
Sakaki, N.
Tameda, Y.
Tsunesada, Y.
Ulrich, A.
dc.subject.por.fl_str_mv astro-ph.HE
astro-ph.IM
topic astro-ph.HE
astro-ph.IM
description 12 pages, 17 figures, 2 tables, International Symposium on Future Directions in UHECR Physics, 13-16 February 2012, CERN, Geneva (Switzerland); the updated version corrects for a typo in Eq. (1)
publishDate 2012
dc.date.none.fl_str_mv 2012-10-04
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/10316/109735
http://hdl.handle.net/10316/109735
https://doi.org/10.1051/epjconf/20135301010
url http://hdl.handle.net/10316/109735
https://doi.org/10.1051/epjconf/20135301010
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 2100-014X
http://arxiv.org/abs/1210.1319v2
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dc.publisher.none.fl_str_mv EDP Sciences
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dc.source.none.fl_str_mv reponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
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