Study of the magnetospheres of active regions on the sun by radio astronomy techniques

摘要: In the 1990s, based on detailed studies of structure active regions (AR), concept magnetosphere region was proposed. This includes almost all known structures presented in region, ranging from radio granulation up to noise storms, radiation which manifests waves. The concept, which, a common point view, considers manifestations emission as single complex, allows one shed light relation between stable and processes their interrelations. It is especially important identify basic ways transforming nonthermal energy into thermal energy. A dominant role attributed magnetic field, measurement coronal levels can be performed by radio-astronomical techniques. extension wavelength range introduction new tools advanced modeling capabilities makes it possible analyze physical properties plasma AR evaluate fields at chromosphere–corona transition zone lower corona. features characteristics S component B have been estimated.