Principle component analysis (PCA) of the solar background magnetic field (SBMF)
measured from Wilcox Solar Observatory (WSO) magnetograms revealed the following …

We have investigated the behavior of dynamo waves within the framework of a nonlinear αω-
dynamo by taking into account the thickness of the convective zone, turbulent diffusivity, and …

Magnetic field generation and evolution models that are capable of describing a large body
of observational material are currently available for different celestial bodies. Despite recent …

В настоящее время разработаны модели генерации и эволюции магнитного поля
Солнца, звёзд и галактик, описывающие большой наблюдательный материал …

The cycles of solar magnetic activity are connected with a solar dynamo that operates in the
convective zone. Solar dynamo mechanism is based on the combined action of the …

Asymptotic methods are used to study a one-dimensional kinematic-Parker dynamo wave
model in the limit when the strength of the-sources, as measured by the dynamo number, is …

A dynamic system for the Parker dynamo including meridional circulation that is applicable
to astrophysical objects is constructed. The meridional circulation is able to control the …

Based on an analysis of the observational data for solar cycles 12–23 (Royal Greenwich
Observatory-USAF/NOAA Sunspot Data), we have studied various parameters of the …

We try to establish the correlation between different parameters of" butterfly-diagrams"
derived from the analysis of solar observational data for the 12-23 solar activity cycles and …

We studied the problem of the behavior of the magnetic field in the case of two-layer
medium. We included of the meridional circulation in this model and investigated the …