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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
dc.description.procedenceUCR::Vicerrectoría de Investigación::Unidades de Investigación::Ciencias Básicas::Centro de Investigaciones Espaciales (CINESPA)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.doihttps://doi.org/10.1017/S1743921313011356
dc.identifier.issn1743-9221
dc.identifier.urihttps://hdl.handle.net/10669/85855
dc.language.isoeng
dc.rightsacceso abierto
dc.sourceProceedings of the International Astronomical Union, vol.8(S300), pp.418-419.es
dc.subjectCoronal holees
dc.subjectProminencees
dc.subjectMagnetic fieldes
dc.subjectCMEes
dc.titleEvolution of a group of coronal holes associated with eruption of nearby prominences and CMEses
dc.typecomunicación de congresoes

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