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On the unusual H∈ emission in a sunspot umbra spectrum
Authors:I P Turova
Institution:(1) Institute of Solar-Terrestrial Physics, 664033 Irkutsk, Russia
Abstract:A study is made of characteristics of the oscillatory process in a sunspot where, in addition to the high brightness in the cores of the H and K Caii lines, the H∈ line was also in emission. A bright H∈ emission persisted during six days at least. An analog of the behaviour of the Caii and H∈ lines can be seen, presumably, on dwarf stars dKe and dMe.
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