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Influence of calcination atmosphere on the phase evolution mechanism of Bi-2223 high temperature superconductor

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Abstract

Precursor powders of Bi2Sr2Ca2Cu3O10+δ (Bi-2223) high temperature superconducting tapes were prepared with spray pyrolysis technique. By tuning the oxygen partial pressure in calcination atmosphere as 1.0%, 7.5%, and 10.0%, respectively, the influences of calcination atmosphere on the phase evolution dynamics during the precursor powders calcination process have been discussed. Then the optimal calcination temperatures have been obtained correspondingly. Moreover, Bi-2223 multi-filament tapes have been fabricated with the precursor powders calcinated under different atmosphere. The effects of precursor powder calcination parameters on the phase composition, microstructures as well as the current capacity of final tapes have been systematically studied. Due to the proper secondary phase content and enhanced Bi-2223 texture structures, the maximum critical current of 109 A at 77 K, self-field, corresponding to the critical current density of 23.3 kA cm−2 has been obtained with the oxygen partial pressure of 7.5% in calcination atmosphere and the calcination temperature of 790 °C.

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Acknowledgements

This study was financially supported by Light of West China under contract No. XAB2018AW15 and the International Cooperative Project in Shaanxi Province, No. 2018kw-055.

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Author notes

  1. Shengnan Zhang and Botao Shao have contributed equally to this work.

Authors and Affiliations

  1. Northwest Institute for Nonferrous Metal Research (NIN), Xi’an, 710016, China

    Shengnan Zhang, Botao Shao, Xiaobo Ma, Jianqing Feng, Xueqian Liu, Chengshan Li & Pingxiang Zhang

  2. Western Superconducting Technology Co., Ltd, Xi’an, 710018, China

    Lijun Cui & Pingxiang Zhang

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  1. Shengnan Zhang
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  2. Botao Shao
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Zhang, S., Shao, B., Ma, X. et al. Influence of calcination atmosphere on the phase evolution mechanism of Bi-2223 high temperature superconductor. J Mater Sci: Mater Electron 31, 12333–12344 (2020). https://doi.org/10.1007/s10854-020-03779-9

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  • DOI: https://doi.org/10.1007/s10854-020-03779-9

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