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dc.contributor.author Cabezas, Denis P.
dc.contributor.author Martínez, Lurdes M.
dc.contributor.author Buleje, Yovanny J.
dc.contributor.author Ishitsuka, Mutsumi
dc.contributor.author Ishitsuka, José K.
dc.contributor.author Morita, Satoshi
dc.contributor.author Asai, Ayumi
dc.contributor.author Ueno, Satoru
dc.contributor.author Ishii, Takato T.
dc.contributor.author Kitai, Reizaburo
dc.contributor.author Takasao, Shinsuke
dc.contributor.author Yoshinaga, Yusuke
dc.contributor.author Otsuji, Kenichi
dc.contributor.author Shibata, Kazunari
dc.date.accessioned 2018-08-03T12:51:37Z
dc.date.available 2018-08-03T12:51:37Z
dc.date.issued 2017-01
dc.identifier.citation Cabezas, D. P., Martínez, L. M., Buleje, Y. J., Ishitsuka, M., Ishitsuka, J. K., Morita, S., ... & Shibata, K. (2017). "Dandelion" filament eruption and coronal waves associated with a solar flare on 2011 February 16.==$The Astrophysical Journal, 836$==(33), 1-11. https://doi.org/10.3847/1538-4357/836/1/33 es_ES
dc.identifier.govdoc index-oti2018
dc.identifier.uri http://hdl.handle.net/20.500.12816/2213
dc.description.abstract Coronal disturbances associated with solar flares, such as Hα Moreton waves, X-ray waves, and extreme ultraviolet (EUV) coronal waves, are discussed herein in relation to magnetohydrodynamic fast-mode waves or shocks in the corona. To understand the mechanism of coronal disturbances, full-disk solar observations with high spatial and temporal resolution over multiple wavelengths are of crucial importance. We observed a filament eruption, whose shape is like a “dandelion,” associated with the M1.6 flare that occurred on 2011 February 16 in Hα images taken by the Flare Monitoring Telescope at Ica University, Peru. We derive the three-dimensional velocity field of the erupting filament. We also identify winking filaments that are located far from the flare site in the Hα images, whereas no Moreton wave is observed. By comparing the temporal evolution of the winking filaments with those of the coronal wave seen in the EUV images data taken by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory and by the Extreme Ultraviolet Imager on board the Solar Terrestrial Relations Observatory-Ahead, we confirm that the winking filaments were activated by the EUV coronal wave. es_ES
dc.format application/pdf es_ES
dc.language.iso eng es_ES
dc.publisher IOP Publishing es_ES
dc.relation.ispartof urn:issn:0004-637X
dc.rights info:eu-repo/semantics/restrictedAccess es_ES
dc.subject Astrophysics es_ES
dc.subject Heliosphere es_ES
dc.subject Solar chromosphere es_ES
dc.subject Sun es_ES
dc.subject Solar magnetic fields es_ES
dc.title "Dandelion" filament eruption and coronal waves associated with a solar flare on 2011 February 16 es_ES
dc.type info:eu-repo/semantics/article es_ES
dc.subject.ocde http://purl.org/pe-repo/ocde/ford#1.05.01 es_ES
dc.identifier.journal The Astrophysical Journal es_ES
dc.description.peer-review Por pares es_ES
dc.identifier.doi https://doi.org/10.3847/1538-4357/836/1/33 es_ES

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