Abstract
In an active region, several points were observed to brighten progressively on the monochromatic image of Hα - 1.2 Å formed by the Domeless Solar Telescope installed recently at Hida Observatory. The phenomena were interpreted as small flares or subflares. The propagation velocity was measured in two cases and discussed in terms of the multiple loop activation observed in EUV radiation.
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References
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Contributions from the Kwasan and Hida Observatories, University of Kyoto, No. 249.
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Kawaguchi, I., Kurokawa, H., Funakoshi, Y. et al. Progressive brightenings observed in the wing of Hα line. Sol Phys 78, 101–105 (1982). https://doi.org/10.1007/BF00151146
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DOI: https://doi.org/10.1007/BF00151146