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- W2024722078 abstract "We present a study of the morphology of quiescent filament observed by H-alpha Solar Telescope at Bosscha Observatory in association with coronal hole observed by Atmospheric Imaging Assembly (AIA) instrument in 193 Å from Solar Dynamics Observatory. H-alpha images were processed by imaging softwares, namely Iris 5.59 and ImageJ, to enhance the signal to noise ratio and to identify the filament features associated with coronal hole. For images observed on October 12, 2011, November 14, 2011 and January 2, 2012, we identified distinct features of coronal holes above the quiescent filaments. This associated coronal holes have filament-like morphology with a thick long thread as it’s ‘spine’, defined as Deep Coronal Hole. Because of strong magnetic field of sunspot, these filaments and coronal holes emerged far from active region and lasted for several days. It is interesting as for segmented filament, deep coronal holes above the filaments lasted for a quite long period of time and merged. This association between filament and deep coronal hole can be explained by filament magnetic loop." @default.
- W2024722078 created "2016-06-24" @default.
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- W2024722078 date "2014-01-01" @default.
- W2024722078 modified "2023-10-12" @default.
- W2024722078 title "Deep coronal hole associated with quiescent filament" @default.
- W2024722078 doi "https://doi.org/10.1063/1.4868738" @default.
- W2024722078 hasPublicationYear "2014" @default.
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