Abstract Samples of high-resolution observations of solar active regions and flares obtained with the 60-cm Domeless Solar Telescope (DST) at Hida Observatory, Kyoto University are presented. What gives rise to the twist and shear in the magnetic loop structures is the essential question for the study of solar active phenomena. Several examples showing the development of twisted or sheared magnetic structures are demonstrated and morphologically studied. Two examples of high-resolution spectra of a flare and spicules are also demonstrated.
High resolution observations of active phenomena obtained at Hida Observatory
Advances in Space Research ; 11 , 5 ; 233-240
1991-01-01
8 pages
Article (Journal)
Electronic Resource
English
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