Trapped field and related properties in a superconducting disk magnetized by pulse field

TL;DR

This paper models magnetic field and temperature distributions in a superconducting disk magnetized by pulse field, analyzing how pulse amplitude affects trapped field and levitation force, with potential applications in magnetic levitation systems.

Contribution

It presents a first-principles calculation of magnetic and thermal distributions in pulse-magnetized superconducting disks, incorporating current dynamics and heat diffusion.

Findings

Trapped magnetic field can reach 17 T at 29 K.

Pulse amplitude significantly influences magnetic field distribution.

Levitation force depends on pulse parameters and temperature.

Abstract

The distributions of the magnetic field and temperature in a superconducting-disk magnetized by pulse field, and the levitation force between this disk and a permanent magnet are calculated from first principles. The calculation is based upon the current motion and the heat diffusion equations in the disk. The critical current density as a function of magnetic field and temperature is taken into account. The dissipation power in the superconducting or the normal state region is distinguished. The trapped field may reach 17 T at 29 K by pulsed field magnetization. The effects of the amplitude of the current pulse on the distributions of magnetic field in the disk and on the levitation force are discussed.