“…For the specified field component, regional S-approximations were constructed: the components of the magnetic induction vector were represented as the sum of simple and double layers, distributed over two or more spheres. In this case, a structural-parametric approach was used: for each of the carriers its own solution vector was determined [8]. In all cases, systems of linear algebraic equations (SLAEs), to which the solution to the inverse problem of restoring the magnetic field of Mercury was reduced, were solved using the Cholesky regularization method and the improved block method for solving SLAEs (for details, see [8]).…”