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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/214691
Ver los metadatos del registro completo
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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 Técnicas2025-09-29T09:39:54Zoai: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:34982025-09-29 09:39:54.787CONICET 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 |
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1844613262593753088 |
score |
13.070432 |