This paper is available on arxiv under CC 4.0 license.
Authors:
(1) A. V. Kuzin, Sternberg Astronomical Institute, Moscow, Russia and E-mail: alv.kuzin@gmail.com.
Table of Links
Model of Disk and Neutron Star
The Solution for the Induced Field
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: