This paper is available on arxiv under CC 4.0 license.

Authors:

(1) A. V. Kuzin, Sternberg Astronomical Institute, Moscow, Russia and E-mail: [email protected].

Abstract and Introduction

Model of Disk and Neutron Star

Main Equations

The Solution for the Induced Field

Discussion

Conclusion and References

2. MODEL OF DISK AND NEUTRON STAR

The magnetic field is assumed to consist of dipolar components that have penetrated the disk and an additional toroidal field: