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.
KeywordsSunspot Group Solar Limb Doppler Width Quiescent Prominence Noise Storm
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