Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments

Autores
Tueros, Matias Jorge; Cabana Freire, Sergio; Álvarez Muñiz, Jaime
Año de publicación
2025
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Atmosphere-skimming air showers are initiated by cosmic rays with incoming directions that allow the cascade to develop entirely within the atmosphere, without reaching the ground. Radio pulses induced by this type of showers have already been observed in balloon-borne experiments such as ANITA, but a detailed characterisation of their properties is lacking. The extreme range of densities in which these cascades can develop gives rise to a wide range of shower profiles, with radio emission characteristics that can differ significantly from those of regular downward-going showers. In this work, we have used the ZHAireS-RASPASS program to characterise the expected radio emission from atmosphere-skimming air showers and its properties. We have studied the interplay between the magnetic field and atmospheric density profile in the expected radio signal, focusing on its detection aboard balloon-borne experiments. The almost horizontal geometry of the events gives rise to a significant refractive asymmetry in the spatial distribution of the electric field, due to the propagation of the radio signals across a gradient of index of refraction. In addition, a unique coherence asymmetry appears in the intensity of the signals, as a consequence of the cumulative effect of the Earth´s magnetic field over the very long distances that these particle cascades traverse. The implications of the peculiar characteristics of the emission are discussed regarding their impact both on the interpretation of collected data and in the exposure of balloon-borne experiments.
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Cabana Freire, Sergio. Universidad de Santiago de Compostela. Facultad de Física; España
Fil: Álvarez Muñiz, Jaime. Universidad de Santiago de Compostela. Facultad de Física; España
Materia
atmosphere-skimming
cosmic ray showers
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:11336/281116

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spelling Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experimentsTueros, Matias JorgeCabana Freire, SergioÁlvarez Muñiz, Jaimeatmosphere-skimmingcosmic ray showersradio detectionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Atmosphere-skimming air showers are initiated by cosmic rays with incoming directions that allow the cascade to develop entirely within the atmosphere, without reaching the ground. Radio pulses induced by this type of showers have already been observed in balloon-borne experiments such as ANITA, but a detailed characterisation of their properties is lacking. The extreme range of densities in which these cascades can develop gives rise to a wide range of shower profiles, with radio emission characteristics that can differ significantly from those of regular downward-going showers. In this work, we have used the ZHAireS-RASPASS program to characterise the expected radio emission from atmosphere-skimming air showers and its properties. We have studied the interplay between the magnetic field and atmospheric density profile in the expected radio signal, focusing on its detection aboard balloon-borne experiments. The almost horizontal geometry of the events gives rise to a significant refractive asymmetry in the spatial distribution of the electric field, due to the propagation of the radio signals across a gradient of index of refraction. In addition, a unique coherence asymmetry appears in the intensity of the signals, as a consequence of the cumulative effect of the Earth´s magnetic field over the very long distances that these particle cascades traverse. The implications of the peculiar characteristics of the emission are discussed regarding their impact both on the interpretation of collected data and in the exposure of balloon-borne experiments.Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Cabana Freire, Sergio. Universidad de Santiago de Compostela. Facultad de Física; EspañaFil: Álvarez Muñiz, Jaime. Universidad de Santiago de Compostela. Facultad de Física; EspañaIOP Publishing2025-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/281116Tueros, Matias Jorge; Cabana Freire, Sergio; Álvarez Muñiz, Jaime; Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2025; 01; 1-2025; 1-231475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2025/01/112info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2025/01/112info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-02-11T12:34:43Zoai:ri.conicet.gov.ar:11336/281116instacron: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:34982026-02-11 12:34:43.58CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
title Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
spellingShingle Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
Tueros, Matias Jorge
atmosphere-skimming
cosmic ray showers
radio detection
title_short Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
title_full Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
title_fullStr Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
title_full_unstemmed Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
title_sort Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments
dc.creator.none.fl_str_mv Tueros, Matias Jorge
Cabana Freire, Sergio
Álvarez Muñiz, Jaime
author Tueros, Matias Jorge
author_facet Tueros, Matias Jorge
Cabana Freire, Sergio
Álvarez Muñiz, Jaime
author_role author
author2 Cabana Freire, Sergio
Álvarez Muñiz, Jaime
author2_role author
author
dc.subject.none.fl_str_mv atmosphere-skimming
cosmic ray showers
radio detection
topic atmosphere-skimming
cosmic ray showers
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 Atmosphere-skimming air showers are initiated by cosmic rays with incoming directions that allow the cascade to develop entirely within the atmosphere, without reaching the ground. Radio pulses induced by this type of showers have already been observed in balloon-borne experiments such as ANITA, but a detailed characterisation of their properties is lacking. The extreme range of densities in which these cascades can develop gives rise to a wide range of shower profiles, with radio emission characteristics that can differ significantly from those of regular downward-going showers. In this work, we have used the ZHAireS-RASPASS program to characterise the expected radio emission from atmosphere-skimming air showers and its properties. We have studied the interplay between the magnetic field and atmospheric density profile in the expected radio signal, focusing on its detection aboard balloon-borne experiments. The almost horizontal geometry of the events gives rise to a significant refractive asymmetry in the spatial distribution of the electric field, due to the propagation of the radio signals across a gradient of index of refraction. In addition, a unique coherence asymmetry appears in the intensity of the signals, as a consequence of the cumulative effect of the Earth´s magnetic field over the very long distances that these particle cascades traverse. The implications of the peculiar characteristics of the emission are discussed regarding their impact both on the interpretation of collected data and in the exposure of balloon-borne experiments.
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Cabana Freire, Sergio. Universidad de Santiago de Compostela. Facultad de Física; España
Fil: Álvarez Muñiz, Jaime. Universidad de Santiago de Compostela. Facultad de Física; España
description Atmosphere-skimming air showers are initiated by cosmic rays with incoming directions that allow the cascade to develop entirely within the atmosphere, without reaching the ground. Radio pulses induced by this type of showers have already been observed in balloon-borne experiments such as ANITA, but a detailed characterisation of their properties is lacking. The extreme range of densities in which these cascades can develop gives rise to a wide range of shower profiles, with radio emission characteristics that can differ significantly from those of regular downward-going showers. In this work, we have used the ZHAireS-RASPASS program to characterise the expected radio emission from atmosphere-skimming air showers and its properties. We have studied the interplay between the magnetic field and atmospheric density profile in the expected radio signal, focusing on its detection aboard balloon-borne experiments. The almost horizontal geometry of the events gives rise to a significant refractive asymmetry in the spatial distribution of the electric field, due to the propagation of the radio signals across a gradient of index of refraction. In addition, a unique coherence asymmetry appears in the intensity of the signals, as a consequence of the cumulative effect of the Earth´s magnetic field over the very long distances that these particle cascades traverse. The implications of the peculiar characteristics of the emission are discussed regarding their impact both on the interpretation of collected data and in the exposure of balloon-borne experiments.
publishDate 2025
dc.date.none.fl_str_mv 2025-01
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/281116
Tueros, Matias Jorge; Cabana Freire, Sergio; Álvarez Muñiz, Jaime; Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2025; 01; 1-2025; 1-23
1475-7516
CONICET Digital
CONICET
url http://hdl.handle.net/11336/281116
identifier_str_mv Tueros, Matias Jorge; Cabana Freire, Sergio; Álvarez Muñiz, Jaime; Radio emission from atmosphere-skimming cosmic ray showers in high-altitude balloon-borne experiments; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2025; 01; 1-2025; 1-23
1475-7516
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2025/01/112
info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2025/01/112
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.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
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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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