Large-scale brightenings associated with flares

Flare-associated large-scale (>1010 cm) X-ray brightenings, the so-called 'giant arches' in the nomenclature of Švestka and co-workers, were discovered in images obtained by the SMM Hard X-ray Imaging Spectrometer hours after the onset of two-ribbon flares. The apparent correlation...

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Autores principales: Mandrini, C.H., Machado, M.E.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00380938_v141_n1_p147_Mandrini
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spelling todo:paper_00380938_v141_n1_p147_Mandrini2023-10-03T14:48:25Z Large-scale brightenings associated with flares Mandrini, C.H. Machado, M.E. Flare-associated large-scale (>1010 cm) X-ray brightenings, the so-called 'giant arches' in the nomenclature of Švestka and co-workers, were discovered in images obtained by the SMM Hard X-ray Imaging Spectrometer hours after the onset of two-ribbon flares. The apparent correlation between both phenomena suggested that they could be interpreted in the framework of the same model. In this paper we show that large-scale loop brightenings, of sizes similar to the giant arches, occur also in association with confined flares in complex active regions. In these cases, the relation between the large-scale structure and the underlying flare is clearly given by the magnetic field topology. We also show that energization of these structures can be partially due to the injection of suprathermal particles that are accelerated at the separator region. We discuss the implications of these results within the framework of the interacting loops picture of flares and of the giant arch phenomenology. © 1992 Kluwer Academic Publishers. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00380938_v141_n1_p147_Mandrini
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description Flare-associated large-scale (>1010 cm) X-ray brightenings, the so-called 'giant arches' in the nomenclature of Švestka and co-workers, were discovered in images obtained by the SMM Hard X-ray Imaging Spectrometer hours after the onset of two-ribbon flares. The apparent correlation between both phenomena suggested that they could be interpreted in the framework of the same model. In this paper we show that large-scale loop brightenings, of sizes similar to the giant arches, occur also in association with confined flares in complex active regions. In these cases, the relation between the large-scale structure and the underlying flare is clearly given by the magnetic field topology. We also show that energization of these structures can be partially due to the injection of suprathermal particles that are accelerated at the separator region. We discuss the implications of these results within the framework of the interacting loops picture of flares and of the giant arch phenomenology. © 1992 Kluwer Academic Publishers.
format JOUR
author Mandrini, C.H.
Machado, M.E.
spellingShingle Mandrini, C.H.
Machado, M.E.
Large-scale brightenings associated with flares
author_facet Mandrini, C.H.
Machado, M.E.
author_sort Mandrini, C.H.
title Large-scale brightenings associated with flares
title_short Large-scale brightenings associated with flares
title_full Large-scale brightenings associated with flares
title_fullStr Large-scale brightenings associated with flares
title_full_unstemmed Large-scale brightenings associated with flares
title_sort large-scale brightenings associated with flares
url http://hdl.handle.net/20.500.12110/paper_00380938_v141_n1_p147_Mandrini
work_keys_str_mv AT mandrinich largescalebrighteningsassociatedwithflares
AT machadome largescalebrighteningsassociatedwithflares
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