In solar facular regions (plages), three distinct classes of magnetic features are observed:
small-scale flux tubes, knots, and pores. Small flux tubes have granular scales; they are in …

Aims. Long-period quasi-periodic variations of the average magnetic field in a small-scale
magnetic structure on the Sun are analysed. The structure is situated at the photospheric …

Quasi-periodical variations in the magnetic fields of long-living, small-scale magnetic
structures, solar facular formations (FFs), are analyzed. We used the method of Empirical …

On 21 September 2012, we carried out spectral observations of a solar facula in the Si i
10827 Å, He i 10830 Å, and H α \upalpha spectral lines. Later, in the process of analyzing …

We studied oscillations related to flare SOL2012-09-21T02: 19 in the transition region and
chromosphere based on Reuven Ramaty High Energy Solar Spectroscopic Imager …

We have studied oscillation processes in the quiet Sun outside a coronal hole at different
levels of the solar chromosphere. The study was based on spectroscopic observations of …

In an effort to detect torsional oscillations, we have studied the periodic half-width variations
for several spectral lines in solar faculae. The duration of the series being analyzed was …

We study Ca ii K profiles in structural features of the quiet chromosphere and plages using
observations of two time series for two regions at the base of a coronal hole. One of the …

С целью обнаружения крутильных колебаний выполнены исследования периодических
вариаций полуширины нескольких спектральных линий в солнечных факелах …

The aim of this paper is to structure and extend the knowledge of solar chromospheric
sources of oscillations in the solar wind and their relationships with pulsations registered in …