Different stages of evolution of prominence and the associated CMEs

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dc.creatorTaliashvili Enacolopas, Lela
dc.creatorMouradian, Zadig
dc.creatorGutiérrez Garro, Heidy
dc.date.accessioned2022-02-03T20:49:15Z
dc.date.available2022-02-03T20:49:15Z
dc.date.issued2013
dc.description.abstractWe study the different evolutional stages of a large quiescent prominence, mainly considering its dynamic/thermal instabilities occurred close from the boundary of coronal hole (CH). We identify the critical conditions, such as the minimum distance between the CH’s boundary and prominence channel and the emergence of a new magnetic flux linked to the prominence instability and its general evolution in connection to CH. Our observations indicate peculiar filament activations prior to its thermal/dynamic instabilities, suggesting the connection of nearby CH with the general evolution of prominence and vice versa. Additionally, we analyze each evolutional stage of prominence and the associated Coronal Mass Ejections (CMEs).es_ES
dc.description.procedenceUCR::Vicerrectoría de Investigación::Unidades de Investigación::Ciencias Básicas::Centro de Investigaciones Espaciales (CINESPA)es_ES
dc.description.sponsorshipInternational Astronomical Union/[]/IAU/Estados Unidoses_ES
dc.identifier.citationhttps://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/different-stages-of-evolution-of-prominence-and-the-associated-cmes/7C41B0702BC22741F6422F071F22F83C
dc.identifier.doi10.1017/S1743921313011721
dc.identifier.issn1743-9221
dc.identifier.urihttps://hdl.handle.net/10669/85673
dc.language.isoenges_ES
dc.rightsacceso abierto
dc.sourceProceedings of the International Astronomical Union, vol.8(S300), pp.497-499.es_ES
dc.subjectProminencees_ES
dc.subjectCoronal holees_ES
dc.subjectCoronal mass ejectiones_ES
dc.subjectMagnetic fluxes_ES
dc.subjectMagnetic fieldes_ES
dc.titleDifferent stages of evolution of prominence and the associated CMEses_ES
dc.typeartículo originales_ES

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