A Burst with Double Radio Spectrum Observed up to 212 GHz

Autores
Gimenez de Castro, C. G.; Cristiani, Germán Diego; Simoes, P. J. A.; Mandrini, Cristina Hemilse; Correia, E.; Kaufmann, P.
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We study a solar flare that occurred on 10 September 2002, in active region NOAA 10105, starting around 14:52 UT and lasting approximately 5 minutes in the radio range. The event was classified as M2.9 in X-rays and 1N in Hα. Solar Submillimeter Telescope observations, in addition to microwave data, give a good spectral coverage between 1.415 and 212 GHz. We combine these data with ultraviolet images, hard and soft X-ray observations, and full-disk magnetograms. Images obtained from Ramaty High Energy Solar Spectroscopic Imager data are used to identify the locations of X-ray sources at different energies, and to determine the X-ray spectrum, while ultraviolet images allow us to characterize the coronal flaring region. The magnetic field evolution of the active region is analyzed using Michelson Doppler Imager magnetograms. The burst is detected at all available radio frequencies. X-ray images (between 12 keV and 300 keV) reveal two compact sources. In the 212 GHz data, which are used to estimate the radio-source position, a single compact source is seen, displaced by 25″ from one of the hard X-ray footpoints. We model the radio spectra using two homogeneous sources, and we combine this analysis with that of hard X-rays to understand the dynamics of the accelerated particles. Relativistic particles, observed at radio wavelengths above 50 GHz, have an electron index evolving with the typical soft–hard–soft behavior.
Fil: Gimenez de Castro, C. G.. CRAAM, Universidade Presbiteriana Mackenzie; Brasil. Consejo Nacional de Investigaciónes 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
Fil: Cristiani, Germán Diego. Consejo Nacional de Investigaciónes 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
Fil: Simoes, P. J. A.. University Of Glasgow; Reino Unido
Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes 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
Fil: Correia, E.. Universidade Presbiteriana Mackenzie; Brasil. Centro de Previsao de Tempo e Estudos Climaticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: Kaufmann, P.. Universidade Presbiteriana Mackenzie; Brasil. Universidade Estadual de Campinas; Brasil
Materia
Radio Bursts, Association with Flares
Microwave Bursts
X-Ray Bursts
Flares, Relation to Magnetic Fields
Chromosphere, Active
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:11336/17087
Acceder
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repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A Burst with Double Radio Spectrum Observed up to 212 GHzGimenez de Castro, C. G.Cristiani, Germán DiegoSimoes, P. J. A.Mandrini, Cristina HemilseCorreia, E.Kaufmann, P.Radio Bursts, Association with FlaresMicrowave BurstsX-Ray BurstsFlares, Relation to Magnetic FieldsChromosphere, Activehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study a solar flare that occurred on 10 September 2002, in active region NOAA 10105, starting around 14:52 UT and lasting approximately 5 minutes in the radio range. The event was classified as M2.9 in X-rays and 1N in Hα. Solar Submillimeter Telescope observations, in addition to microwave data, give a good spectral coverage between 1.415 and 212 GHz. We combine these data with ultraviolet images, hard and soft X-ray observations, and full-disk magnetograms. Images obtained from Ramaty High Energy Solar Spectroscopic Imager data are used to identify the locations of X-ray sources at different energies, and to determine the X-ray spectrum, while ultraviolet images allow us to characterize the coronal flaring region. The magnetic field evolution of the active region is analyzed using Michelson Doppler Imager magnetograms. The burst is detected at all available radio frequencies. X-ray images (between 12 keV and 300 keV) reveal two compact sources. In the 212 GHz data, which are used to estimate the radio-source position, a single compact source is seen, displaced by 25″ from one of the hard X-ray footpoints. We model the radio spectra using two homogeneous sources, and we combine this analysis with that of hard X-rays to understand the dynamics of the accelerated particles. Relativistic particles, observed at radio wavelengths above 50 GHz, have an electron index evolving with the typical soft–hard–soft behavior.Fil: Gimenez de Castro, C. G.. CRAAM, Universidade Presbiteriana Mackenzie; Brasil. Consejo Nacional de Investigaciónes 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; ArgentinaFil: Cristiani, Germán Diego. Consejo Nacional de Investigaciónes 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; ArgentinaFil: Simoes, P. J. A.. University Of Glasgow; Reino UnidoFil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes 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; ArgentinaFil: Correia, E.. Universidade Presbiteriana Mackenzie; Brasil. Centro de Previsao de Tempo e Estudos Climaticos. Instituto Nacional de Pesquisas Espaciais; BrasilFil: Kaufmann, P.. Universidade Presbiteriana Mackenzie; Brasil. Universidade Estadual de Campinas; BrasilSpringer2013-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/17087Gimenez de Castro, C. G.; Cristiani, Germán Diego; Simoes, P. J. A.; Mandrini, Cristina Hemilse; Correia, E.; et al.; A Burst with Double Radio Spectrum Observed up to 212 GHz; Springer; Solar Physics; 284; 2; 6-2013; 541-5580038-0938enginfo:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-012-0173-8info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1208.5904info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs11207-012-0173-8info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:36:21Zoai:ri.conicet.gov.ar:11336/17087instacron: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 09:36:22.154CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A Burst with Double Radio Spectrum Observed up to 212 GHz
title A Burst with Double Radio Spectrum Observed up to 212 GHz
spellingShingle A Burst with Double Radio Spectrum Observed up to 212 GHz
Gimenez de Castro, C. G.
Radio Bursts, Association with Flares
Microwave Bursts
X-Ray Bursts
Flares, Relation to Magnetic Fields
Chromosphere, Active
title_short A Burst with Double Radio Spectrum Observed up to 212 GHz
title_full A Burst with Double Radio Spectrum Observed up to 212 GHz
title_fullStr A Burst with Double Radio Spectrum Observed up to 212 GHz
title_full_unstemmed A Burst with Double Radio Spectrum Observed up to 212 GHz
title_sort A Burst with Double Radio Spectrum Observed up to 212 GHz
dc.creator.none.fl_str_mv Gimenez de Castro, C. G.
Cristiani, Germán Diego
Simoes, P. J. A.
Mandrini, Cristina Hemilse
Correia, E.
Kaufmann, P.
author Gimenez de Castro, C. G.
author_facet Gimenez de Castro, C. G.
Cristiani, Germán Diego
Simoes, P. J. A.
Mandrini, Cristina Hemilse
Correia, E.
Kaufmann, P.
author_role author
author2 Cristiani, Germán Diego
Simoes, P. J. A.
Mandrini, Cristina Hemilse
Correia, E.
Kaufmann, P.
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Radio Bursts, Association with Flares
Microwave Bursts
X-Ray Bursts
Flares, Relation to Magnetic Fields
Chromosphere, Active
topic Radio Bursts, Association with Flares
Microwave Bursts
X-Ray Bursts
Flares, Relation to Magnetic Fields
Chromosphere, Active
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 study a solar flare that occurred on 10 September 2002, in active region NOAA 10105, starting around 14:52 UT and lasting approximately 5 minutes in the radio range. The event was classified as M2.9 in X-rays and 1N in Hα. Solar Submillimeter Telescope observations, in addition to microwave data, give a good spectral coverage between 1.415 and 212 GHz. We combine these data with ultraviolet images, hard and soft X-ray observations, and full-disk magnetograms. Images obtained from Ramaty High Energy Solar Spectroscopic Imager data are used to identify the locations of X-ray sources at different energies, and to determine the X-ray spectrum, while ultraviolet images allow us to characterize the coronal flaring region. The magnetic field evolution of the active region is analyzed using Michelson Doppler Imager magnetograms. The burst is detected at all available radio frequencies. X-ray images (between 12 keV and 300 keV) reveal two compact sources. In the 212 GHz data, which are used to estimate the radio-source position, a single compact source is seen, displaced by 25″ from one of the hard X-ray footpoints. We model the radio spectra using two homogeneous sources, and we combine this analysis with that of hard X-rays to understand the dynamics of the accelerated particles. Relativistic particles, observed at radio wavelengths above 50 GHz, have an electron index evolving with the typical soft–hard–soft behavior.
Fil: Gimenez de Castro, C. G.. CRAAM, Universidade Presbiteriana Mackenzie; Brasil. Consejo Nacional de Investigaciónes 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
Fil: Cristiani, Germán Diego. Consejo Nacional de Investigaciónes 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
Fil: Simoes, P. J. A.. University Of Glasgow; Reino Unido
Fil: Mandrini, Cristina Hemilse. Consejo Nacional de Investigaciónes 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
Fil: Correia, E.. Universidade Presbiteriana Mackenzie; Brasil. Centro de Previsao de Tempo e Estudos Climaticos. Instituto Nacional de Pesquisas Espaciais; Brasil
Fil: Kaufmann, P.. Universidade Presbiteriana Mackenzie; Brasil. Universidade Estadual de Campinas; Brasil
description We study a solar flare that occurred on 10 September 2002, in active region NOAA 10105, starting around 14:52 UT and lasting approximately 5 minutes in the radio range. The event was classified as M2.9 in X-rays and 1N in Hα. Solar Submillimeter Telescope observations, in addition to microwave data, give a good spectral coverage between 1.415 and 212 GHz. We combine these data with ultraviolet images, hard and soft X-ray observations, and full-disk magnetograms. Images obtained from Ramaty High Energy Solar Spectroscopic Imager data are used to identify the locations of X-ray sources at different energies, and to determine the X-ray spectrum, while ultraviolet images allow us to characterize the coronal flaring region. The magnetic field evolution of the active region is analyzed using Michelson Doppler Imager magnetograms. The burst is detected at all available radio frequencies. X-ray images (between 12 keV and 300 keV) reveal two compact sources. In the 212 GHz data, which are used to estimate the radio-source position, a single compact source is seen, displaced by 25″ from one of the hard X-ray footpoints. We model the radio spectra using two homogeneous sources, and we combine this analysis with that of hard X-rays to understand the dynamics of the accelerated particles. Relativistic particles, observed at radio wavelengths above 50 GHz, have an electron index evolving with the typical soft–hard–soft behavior.
publishDate 2013
dc.date.none.fl_str_mv 2013-06
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/11336/17087
Gimenez de Castro, C. G.; Cristiani, Germán Diego; Simoes, P. J. A.; Mandrini, Cristina Hemilse; Correia, E.; et al.; A Burst with Double Radio Spectrum Observed up to 212 GHz; Springer; Solar Physics; 284; 2; 6-2013; 541-558
0038-0938
url http://hdl.handle.net/11336/17087
identifier_str_mv Gimenez de Castro, C. G.; Cristiani, Germán Diego; Simoes, P. J. A.; Mandrini, Cristina Hemilse; Correia, E.; et al.; A Burst with Double Radio Spectrum Observed up to 212 GHz; Springer; Solar Physics; 284; 2; 6-2013; 541-558
0038-0938
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1007/s11207-012-0173-8
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/1208.5904
info:eu-repo/semantics/altIdentifier/url/https://link.springer.com/article/10.1007%2Fs11207-012-0173-8
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
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
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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