Properties of fast submillimeter time structures during a large solar flare

Autores
Raulin, Jean Pierre; Kaufmann, Pierre; de Castro, Carlos G. Giménez; Pacini, Alessandra A.; Makhmutov, Vladimir S.; Levato, Orlando Hugo; Rovira, Marta Graciela
Año de publicación
2003
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We report properties of fast varying submillimeter emission during one of the strongest solar radio flares of solar cycle 23. Emission was obtained by the Solar Submillimeter-Wave Telescope at 212 and 405 GHz and compared with hard X-ray and γ-ray counts up to few tens of MeV photon energy ranges. We employ different methods to detect and characterize flux density variations and find that during the impulsive phase of the event, the closer in time to the peak flare, the higher the occurrence of the fastest and brightest time structures. The good comparison with hard X-ray and γ-ray count rates indicates that fast submillimeter pulses are the signatures of primary energetic injections. The characteristics of the fast spikes at 212 and 405 GHz, such as their flux density and localization, compared to those of the underlying slower impulsive component, also suggest that their nature is different.
Fil: Raulin, Jean Pierre. Universidade Presbiteriana Mackenzie; Brasil
Fil: Kaufmann, Pierre. Universidade Estadual de Campinas; Brasil. Universidade Presbiteriana Mackenzie; Brasil
Fil: de Castro, Carlos G. Giménez. Universidade Presbiteriana Mackenzie; Brasil
Fil: Pacini, Alessandra A.. Universidade Presbiteriana Mackenzie; Brasil
Fil: Makhmutov, Vladimir S.. Russian Academy Of Sciences; Rusia
Fil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Rovira, Marta Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Materia
GAMMA RAYS: BURSTS
SUN: FLARES
SUN: RADIO RADIATION
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:11336/214691
Acceder
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Properties of fast submillimeter time structures during a large solar flareRaulin, Jean PierreKaufmann, Pierrede Castro, Carlos G. GiménezPacini, Alessandra A.Makhmutov, Vladimir S.Levato, Orlando HugoRovira, Marta GracielaGAMMA RAYS: BURSTSSUN: FLARESSUN: RADIO RADIATIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We report properties of fast varying submillimeter emission during one of the strongest solar radio flares of solar cycle 23. Emission was obtained by the Solar Submillimeter-Wave Telescope at 212 and 405 GHz and compared with hard X-ray and γ-ray counts up to few tens of MeV photon energy ranges. We employ different methods to detect and characterize flux density variations and find that during the impulsive phase of the event, the closer in time to the peak flare, the higher the occurrence of the fastest and brightest time structures. The good comparison with hard X-ray and γ-ray count rates indicates that fast submillimeter pulses are the signatures of primary energetic injections. The characteristics of the fast spikes at 212 and 405 GHz, such as their flux density and localization, compared to those of the underlying slower impulsive component, also suggest that their nature is different.Fil: Raulin, Jean Pierre. Universidade Presbiteriana Mackenzie; BrasilFil: Kaufmann, Pierre. Universidade Estadual de Campinas; Brasil. Universidade Presbiteriana Mackenzie; BrasilFil: de Castro, Carlos G. Giménez. Universidade Presbiteriana Mackenzie; BrasilFil: Pacini, Alessandra A.. Universidade Presbiteriana Mackenzie; BrasilFil: Makhmutov, Vladimir S.. Russian Academy Of Sciences; RusiaFil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Rovira, Marta Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaIOP Publishing2003-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/214691Raulin, Jean Pierre; Kaufmann, Pierre; de Castro, Carlos G. Giménez; Pacini, Alessandra A.; Makhmutov, Vladimir S.; et al.; Properties of fast submillimeter time structures during a large solar flare; IOP Publishing; Astrophysical Journal; 592; 1 I; 12-2003; 580-5890004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/375718info:eu-repo/semantics/altIdentifier/doi/10.1086/375718info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:29:25Zoai:ri.conicet.gov.ar:11336/214691instacron: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:34982025-10-15 14:29:25.576CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Properties of fast submillimeter time structures during a large solar flare
title Properties of fast submillimeter time structures during a large solar flare
spellingShingle Properties of fast submillimeter time structures during a large solar flare
Raulin, Jean Pierre
GAMMA RAYS: BURSTS
SUN: FLARES
SUN: RADIO RADIATION
title_short Properties of fast submillimeter time structures during a large solar flare
title_full Properties of fast submillimeter time structures during a large solar flare
title_fullStr Properties of fast submillimeter time structures during a large solar flare
title_full_unstemmed Properties of fast submillimeter time structures during a large solar flare
title_sort Properties of fast submillimeter time structures during a large solar flare
dc.creator.none.fl_str_mv Raulin, Jean Pierre
Kaufmann, Pierre
de Castro, Carlos G. Giménez
Pacini, Alessandra A.
Makhmutov, Vladimir S.
Levato, Orlando Hugo
Rovira, Marta Graciela
author Raulin, Jean Pierre
author_facet Raulin, Jean Pierre
Kaufmann, Pierre
de Castro, Carlos G. Giménez
Pacini, Alessandra A.
Makhmutov, Vladimir S.
Levato, Orlando Hugo
Rovira, Marta Graciela
author_role author
author2 Kaufmann, Pierre
de Castro, Carlos G. Giménez
Pacini, Alessandra A.
Makhmutov, Vladimir S.
Levato, Orlando Hugo
Rovira, Marta Graciela
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv GAMMA RAYS: BURSTS
SUN: FLARES
SUN: RADIO RADIATION
topic GAMMA RAYS: BURSTS
SUN: FLARES
SUN: RADIO RADIATION
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We report properties of fast varying submillimeter emission during one of the strongest solar radio flares of solar cycle 23. Emission was obtained by the Solar Submillimeter-Wave Telescope at 212 and 405 GHz and compared with hard X-ray and γ-ray counts up to few tens of MeV photon energy ranges. We employ different methods to detect and characterize flux density variations and find that during the impulsive phase of the event, the closer in time to the peak flare, the higher the occurrence of the fastest and brightest time structures. The good comparison with hard X-ray and γ-ray count rates indicates that fast submillimeter pulses are the signatures of primary energetic injections. The characteristics of the fast spikes at 212 and 405 GHz, such as their flux density and localization, compared to those of the underlying slower impulsive component, also suggest that their nature is different.
Fil: Raulin, Jean Pierre. Universidade Presbiteriana Mackenzie; Brasil
Fil: Kaufmann, Pierre. Universidade Estadual de Campinas; Brasil. Universidade Presbiteriana Mackenzie; Brasil
Fil: de Castro, Carlos G. Giménez. Universidade Presbiteriana Mackenzie; Brasil
Fil: Pacini, Alessandra A.. Universidade Presbiteriana Mackenzie; Brasil
Fil: Makhmutov, Vladimir S.. Russian Academy Of Sciences; Rusia
Fil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Rovira, Marta Graciela. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
description We report properties of fast varying submillimeter emission during one of the strongest solar radio flares of solar cycle 23. Emission was obtained by the Solar Submillimeter-Wave Telescope at 212 and 405 GHz and compared with hard X-ray and γ-ray counts up to few tens of MeV photon energy ranges. We employ different methods to detect and characterize flux density variations and find that during the impulsive phase of the event, the closer in time to the peak flare, the higher the occurrence of the fastest and brightest time structures. The good comparison with hard X-ray and γ-ray count rates indicates that fast submillimeter pulses are the signatures of primary energetic injections. The characteristics of the fast spikes at 212 and 405 GHz, such as their flux density and localization, compared to those of the underlying slower impulsive component, also suggest that their nature is different.
publishDate 2003
dc.date.none.fl_str_mv 2003-12
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/11336/214691
Raulin, Jean Pierre; Kaufmann, Pierre; de Castro, Carlos G. Giménez; Pacini, Alessandra A.; Makhmutov, Vladimir S.; et al.; Properties of fast submillimeter time structures during a large solar flare; IOP Publishing; Astrophysical Journal; 592; 1 I; 12-2003; 580-589
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/214691
identifier_str_mv Raulin, Jean Pierre; Kaufmann, Pierre; de Castro, Carlos G. Giménez; Pacini, Alessandra A.; Makhmutov, Vladimir S.; et al.; Properties of fast submillimeter time structures during a large solar flare; IOP Publishing; Astrophysical Journal; 592; 1 I; 12-2003; 580-589
0004-637X
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/10.1086/375718
info:eu-repo/semantics/altIdentifier/doi/10.1086/375718
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
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)
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
_version_ 1846082764913246208
score 13.22299

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