Localization of the Attractor of the Differential Equations for the Solar Wind–Magnetosphere–Ionosphere Model

摘要

The problem of localization of the attractor of a three-dimensional solar wind–magnetosphere–ionosphere model (the WINDMI model [1, 2]) has stimulated the development of the method of conical nets to solve this problem. In this communication, we describe this development and obtain analytical estimates for the attractor of the model.