4.5 Article

Numerical investigations on the characteristics of thermomagnetic instability in MgB2 bulks

Journal

SUPERCONDUCTOR SCIENCE & TECHNOLOGY
Volume 30, Issue 7, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/1361-6668/aa73b3

Keywords

thermomagnetic instability; flux jump; MgB2 bulks; type-II superconductor; finite element method

Funding

  1. China Postdoctoral Science Foundation [2017M610064]
  2. National Magnetic Confinement Fusion Energy Research Project [2015GB108002]
  3. Innovative Research Group of the National Natural Science Foundation of China [11421062]

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This paper presents the characteristics of thermomagnetic instability in MgB2 bulks by numerically solving the macroscopic dynamics of thermomagnetic interaction governed by the coupled magnetic and heat diffusion equations in association with a modified E - J power-law relationship. The finite element method is used to discretize the system of partial differential equations. The calculated magnetization loops with flux jumps are consistent with the experimental results for MgB2 slabs bathed in a wide range of ambient temperatures. We reveal the evolution process of the thermomagnetic instability and present the distributions of the magnetic field, temperature, and current density before and after flux jumps. A 2D axisymmetric model is used to study the thermomagnetic instability in cylindrical MgB2 bulks. It is found that the number of flux jumps monotonously reduces as the ambient temperature rises and no flux jump appears when the ambient temperature exceeds a certain value. Moreover, the flux-jump phenomenon exists in a wide range of the ramp rate of the applied external field, i.e. 10(-2)-10(2) T s(-1). Furthermore, the dependences of the first flux-jump field on the ambient temperature, ramp rate, and bulk thickness are investigated. The critical bulk thicknesses for stability are obtained for different ambient temperatures and sample radii. In addition, the influence of the capability of the interfacial heat transfer on the temporal response of the bulk temperature is discussed. We also find that the prediction of thermomagnetic instability is sensitive to the employment of the flux creep exponent in the simulations.

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