quadrupole
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Multipole Magnetic Field Lines Interaction of Neutron Stars
Abstract: In this paper, we present the magnetic field of the collapsed core during a massive star supernova explosion, resulting from the conservation of magnetic flux, which forms a strong magnetic fields (B∽1013 G) Neutron stars. The vector potential from moving electric charge Q uniformly distributed over the surface of the spherical Neutron star of radius R and the multipole magnetic field have calculated. The interaction between the dipole magnetic field …
Published in Research & Reviews : Journal of Physics · Vol. 9, Issue 2, 2020 · pp. 6–15 Read article