Height-Dependent Short-Period Oscillations in the Fe XIV (530.3 nm) Solar Corona Above a Sunspot Group Crossing the Limb
A sequence of 86 green coronal line spectra is analyzed in order to find short-period oscillations in the corona. It is shown that a tendency exists of the revealed periods to change with the height above the limb.
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- Tsubaki, T.: 1988, in “Solar and stellar coronal structures and dynamics”, ed. R. C. Altrock, Proc. 9th Sac. Peak Summer Symp., Sunspot, NM, 17–21 Aug 1987, 140.Google Scholar