CAII lines in a quiet region on the Sun I. Dynamic processes in the solar atmosphere

We have studied oscillation processes in the quiet Sun outside a coronal hole at different levels of solar chromosphere. The study was based on spectroscopic observations ionized calcium lines (K, H, and 849.8 nm) obtained by Sayan Solar Observatory’s Automated Telescope (AST). Spectral analysis time series for some parameters has been carried out. compared results this work with our regions located base hole. power found to be higher region At same time, under there is common tendency decrease height all frequency ranges, except low-frequency one, most chromospheric structures. In structures weak magnetic field, increases lower chromosphere decreases somewhat upper