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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.
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Table of Links
Model of Disk and Neutron Star
The Solution for the Induced Field
5. DISCUSSION
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5.1. Axisymmetric component
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5.2. Possible azimuthal-dependent contributions
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It is unclear to what extent the φ-dependent components of the dipolar field penetrate the disk. In case they do not penetrate the disk at all, the induced field is given by b(r, z). Lai (1999) attempted to build a model of the induced field in this scenario (the ”Hybrid model”).
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