Radio morphing: towards a full parametrisation of the radio signal from air showers

Autores
Zilles, A.; Charried, D.; Kotera, K.; Le Coz, S.; Martineau Huynh, O.; Medina, Maria Clementina; Niess, V.; Tueros, Matias Jorge; D. de Vries, K.
Año de publicación
2018
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Over the last decades, radio detection of air showers has been established as a detection technique for ultra-high-energy cosmic-rays impinging on the Earth's atmosphere with energies far beyond LHC energies. Today’s second-generation of digital radio-detection experiments, as e.g. AERA or LOFAR, are becoming competitive in comparison to already standard techniques e.g. fluorescence light detection. Thanks to a detailed understanding of the physics of the radio emission in extensive air showers, simulations of the radio signal are already successfully tested and applied in the reconstruction of cosmic rays. However the limits of the computational power resources are easily reached when it comes to computing electric fields at the numerous positions requested by large or dense antenna arrays. In the case of mountainous areas as e.g. for the GRAND array, where 3D shower simulations are necessary, the problem arises with even stronger acuity. Therefore we developed a full parametrisation of the emitted radio signal on the basis of generic shower simulations which will reduce the simulation time by orders of magnitudes. In this talk we will present this concept after a short introduction to the concept of the radio detection of air-shower induced by cosmic rays.
Fil: Zilles, A.. Sorbonne University; Francia
Fil: Charried, D.. Universite de Nantes; Francia
Fil: Kotera, K.. Sorbonne University; Francia
Fil: Le Coz, S.. Chinese Academy of Sciences; República de China
Fil: Martineau Huynh, O.. Universite de Paris VI; Francia. Université Paris VIII; Francia
Fil: Medina, Maria Clementina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Niess, V.. Universite Blaise Pascal; Francia
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: D. de Vries, K.. Vrije Universiteit Brussel; Bélgica
meeting of the French Society of Astronomy and Astrophysics
Paris
Francia
French Society of Astronomy & Astrophysics
Materia
particle air shower
radio emission
radio detection
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/138589
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Radio morphing: towards a full parametrisation of the radio signal from air showersZilles, A.Charried, D.Kotera, K.Le Coz, S.Martineau Huynh, O.Medina, Maria ClementinaNiess, V.Tueros, Matias JorgeD. de Vries, K.particle air showerradio emissionradio detectionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Over the last decades, radio detection of air showers has been established as a detection technique for ultra-high-energy cosmic-rays impinging on the Earth's atmosphere with energies far beyond LHC energies. Today’s second-generation of digital radio-detection experiments, as e.g. AERA or LOFAR, are becoming competitive in comparison to already standard techniques e.g. fluorescence light detection. Thanks to a detailed understanding of the physics of the radio emission in extensive air showers, simulations of the radio signal are already successfully tested and applied in the reconstruction of cosmic rays. However the limits of the computational power resources are easily reached when it comes to computing electric fields at the numerous positions requested by large or dense antenna arrays. In the case of mountainous areas as e.g. for the GRAND array, where 3D shower simulations are necessary, the problem arises with even stronger acuity. Therefore we developed a full parametrisation of the emitted radio signal on the basis of generic shower simulations which will reduce the simulation time by orders of magnitudes. In this talk we will present this concept after a short introduction to the concept of the radio detection of air-shower induced by cosmic rays.Fil: Zilles, A.. Sorbonne University; FranciaFil: Charried, D.. Universite de Nantes; FranciaFil: Kotera, K.. Sorbonne University; FranciaFil: Le Coz, S.. Chinese Academy of Sciences; República de ChinaFil: Martineau Huynh, O.. Universite de Paris VI; Francia. Université Paris VIII; FranciaFil: Medina, Maria Clementina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaFil: Niess, V.. Universite Blaise Pascal; FranciaFil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: D. de Vries, K.. Vrije Universiteit Brussel; Bélgicameeting of the French Society of Astronomy and AstrophysicsParisFranciaFrench Society of Astronomy & AstrophysicsFrench Society of Astronomy and AstrophysicsReylé, C.Di Matteo, P.Herpin, F.Lagadec, E.Lancon, A.Meliani, Z.Royer, F.2018info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectReuniónBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/138589Radio morphing: towards a full parametrisation of the radio signal from air showers; meeting of the French Society of Astronomy and Astrophysics; Paris; Francia; 2017; 165-168CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://cdsads.u-strasbg.fr/abs/2017sf2a.conf..165Zinfo:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1809.04910info:eu-repo/semantics/altIdentifier/url/http://shorturl.at/yFY01info:eu-repo/semantics/altIdentifier/url/http://sf2a.eu/proceedings/2017/2017sf2a.conf..0165Z.pdfInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:39:27Zoai:ri.conicet.gov.ar:11336/138589instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:39:27.539CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Radio morphing: towards a full parametrisation of the radio signal from air showers
title Radio morphing: towards a full parametrisation of the radio signal from air showers
spellingShingle Radio morphing: towards a full parametrisation of the radio signal from air showers
Zilles, A.
particle air shower
radio emission
radio detection
title_short Radio morphing: towards a full parametrisation of the radio signal from air showers
title_full Radio morphing: towards a full parametrisation of the radio signal from air showers
title_fullStr Radio morphing: towards a full parametrisation of the radio signal from air showers
title_full_unstemmed Radio morphing: towards a full parametrisation of the radio signal from air showers
title_sort Radio morphing: towards a full parametrisation of the radio signal from air showers
dc.creator.none.fl_str_mv Zilles, A.
Charried, D.
Kotera, K.
Le Coz, S.
Martineau Huynh, O.
Medina, Maria Clementina
Niess, V.
Tueros, Matias Jorge
D. de Vries, K.
author Zilles, A.
author_facet Zilles, A.
Charried, D.
Kotera, K.
Le Coz, S.
Martineau Huynh, O.
Medina, Maria Clementina
Niess, V.
Tueros, Matias Jorge
D. de Vries, K.
author_role author
author2 Charried, D.
Kotera, K.
Le Coz, S.
Martineau Huynh, O.
Medina, Maria Clementina
Niess, V.
Tueros, Matias Jorge
D. de Vries, K.
author2_role author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Reylé, C.
Di Matteo, P.
Herpin, F.
Lagadec, E.
Lancon, A.
Meliani, Z.
Royer, F.
dc.subject.none.fl_str_mv particle air shower
radio emission
radio detection
topic particle air shower
radio emission
radio detection
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Over the last decades, radio detection of air showers has been established as a detection technique for ultra-high-energy cosmic-rays impinging on the Earth's atmosphere with energies far beyond LHC energies. Today’s second-generation of digital radio-detection experiments, as e.g. AERA or LOFAR, are becoming competitive in comparison to already standard techniques e.g. fluorescence light detection. Thanks to a detailed understanding of the physics of the radio emission in extensive air showers, simulations of the radio signal are already successfully tested and applied in the reconstruction of cosmic rays. However the limits of the computational power resources are easily reached when it comes to computing electric fields at the numerous positions requested by large or dense antenna arrays. In the case of mountainous areas as e.g. for the GRAND array, where 3D shower simulations are necessary, the problem arises with even stronger acuity. Therefore we developed a full parametrisation of the emitted radio signal on the basis of generic shower simulations which will reduce the simulation time by orders of magnitudes. In this talk we will present this concept after a short introduction to the concept of the radio detection of air-shower induced by cosmic rays.
Fil: Zilles, A.. Sorbonne University; Francia
Fil: Charried, D.. Universite de Nantes; Francia
Fil: Kotera, K.. Sorbonne University; Francia
Fil: Le Coz, S.. Chinese Academy of Sciences; República de China
Fil: Martineau Huynh, O.. Universite de Paris VI; Francia. Université Paris VIII; Francia
Fil: Medina, Maria Clementina. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Fil: Niess, V.. Universite Blaise Pascal; Francia
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: D. de Vries, K.. Vrije Universiteit Brussel; Bélgica
meeting of the French Society of Astronomy and Astrophysics
Paris
Francia
French Society of Astronomy & Astrophysics
description Over the last decades, radio detection of air showers has been established as a detection technique for ultra-high-energy cosmic-rays impinging on the Earth's atmosphere with energies far beyond LHC energies. Today’s second-generation of digital radio-detection experiments, as e.g. AERA or LOFAR, are becoming competitive in comparison to already standard techniques e.g. fluorescence light detection. Thanks to a detailed understanding of the physics of the radio emission in extensive air showers, simulations of the radio signal are already successfully tested and applied in the reconstruction of cosmic rays. However the limits of the computational power resources are easily reached when it comes to computing electric fields at the numerous positions requested by large or dense antenna arrays. In the case of mountainous areas as e.g. for the GRAND array, where 3D shower simulations are necessary, the problem arises with even stronger acuity. Therefore we developed a full parametrisation of the emitted radio signal on the basis of generic shower simulations which will reduce the simulation time by orders of magnitudes. In this talk we will present this concept after a short introduction to the concept of the radio detection of air-shower induced by cosmic rays.
publishDate 2018
dc.date.none.fl_str_mv 2018
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Reunión
Book
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/138589
Radio morphing: towards a full parametrisation of the radio signal from air showers; meeting of the French Society of Astronomy and Astrophysics; Paris; Francia; 2017; 165-168
CONICET Digital
CONICET
url http://hdl.handle.net/11336/138589
identifier_str_mv Radio morphing: towards a full parametrisation of the radio signal from air showers; meeting of the French Society of Astronomy and Astrophysics; Paris; Francia; 2017; 165-168
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://cdsads.u-strasbg.fr/abs/2017sf2a.conf..165Z
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1809.04910
info:eu-repo/semantics/altIdentifier/url/http://shorturl.at/yFY01
info:eu-repo/semantics/altIdentifier/url/http://sf2a.eu/proceedings/2017/2017sf2a.conf..0165Z.pdf
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv French Society of Astronomy and Astrophysics
publisher.none.fl_str_mv French Society of Astronomy and Astrophysics
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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