STRUCTURE AND DYNAMICS OF PLASMA FORMATIONS IN THE SUN`S ATMOSPHERE IN THE PHASE EVOLUTION OF SOLAR ACTIVITY
Year: 2025

The plasma formations in the solar atmosphere, observed in white light (the so-called continuum) and in different spectral lines, reflect the structure of the magnetic field, the dynamics of which generate all solar activity. Thus, although the magnetic field in the corona cannot yet be accurately measured, the plasma structures outline the magnetic field lines and even provide information about the electric currents flowing in the corona. The report compares the general shape of the white coron