Evolution of a group of coronal holes associated with eruption of nearby prominences and CMEs

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dc.creatorGutiérrez Garro, Heidy
dc.creatorTaliashvili Enacolopas, Lela
dc.creatorMouradian, Zadig
dc.date.accessioned2022-02-25T14:17:39Z
dc.date.available2022-02-25T14:17:39Z
dc.date.issued2014-01-06
dc.description.abstractWe present the results of detailed study of a set of activities developed on one of three enclosed sectors of solar region during the period of February 07-13, 2012. We found the sequence of certain topological perturbations of whole coronal holes (CHs) and their surroundings associated to the eruption of nearby prominence and subsequent Coronal Mass Ejections (CMEs). Especially, we observe the emergence of small bright points (BPs) and the formation of dimming regions (DRs) close to the filament's channel associated with a pre-evolution of filament/prominence eruption, whereas BPs disappearance and the shrinkage of CH we found associated with the post-eruption evolution of prominence and of CME.es_ES
dc.description.procedenceUCR::Vicerrectoría de Investigación::Unidades de Investigación::Ciencias Básicas::Centro de Investigaciones Espaciales (CINESPA)es_ES
dc.identifier.citationhttps://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/evolution-of-a-group-of-coronal-holes-associated-with-eruption-of-nearby-prominences-and-cmes/30D3A13EA1CB1C39A19D179237D2555F
dc.identifier.doi10.1017/S1743921313011356
dc.identifier.issn1743-9221
dc.identifier.urihttps://hdl.handle.net/10669/85855
dc.language.isoenges_ES
dc.rightsacceso abierto
dc.sourceProceedings of the International Astronomical Union, vol.8(S300), pp.418-419.es_ES
dc.subjectCoronal holees_ES
dc.subjectProminencees_ES
dc.subjectMagnetic fieldes_ES
dc.subjectCMEes_ES
dc.titleEvolution of a group of coronal holes associated with eruption of nearby prominences and CMEses_ES
dc.typecomunicación de congresoes_ES

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