Magnetization behavior of RE123 bulk magnets bearing twin seed-crystals in pulsed field magnetization processes
Magnetization behavior of RE123 bulk magnets bearing twin seed-crystals in pulsed field magnetization processes
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脉冲场磁化过程中带有孪晶的 RE123 块体磁体的磁化行为
DOI:
10.1088/0953-2048/29/2/024003
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发表时间:
2016
影响因子:
3.6
通讯作者:
K. Yokoyama
中科院分区:
文献类型:
--
作者:
T. Oka;T. Miyazaki;J. Ogawa;S. Fukui;T. Sato;K. Yokoyama
Melt-textured Y-Ba-Cu-O high temperature superconducting bulk magnets were fabricated by the cold seeding method with using single or twin-seed crystals composed of Nd-Ba-Cu-O thin films on MgO substrates. The behavior of the magnetic flux penetration into anisotropic-grown bulk magnets thus fabricated was precisely evaluated during and after the pulsed field magnetization operated at 35 K. These seed crystals were put on the top surfaces of the precursors to grow large grains during the melt-processes. Although we know the magnetic flux motion is restricted by the enhanced pinning effect in temperature ranges lower than 77 K, we observed that flux invasion occurred at applied fields of 3.3 T when the twin seeds were used. This is definitely lower than those of 3.7 T when the single-seeds were employed. This means that the magnetic fluxes are capable of invading into twin-seeded bulk magnets more easily than single-seeded ones. The twin seeds form the different grain growth regions, the narrow-GSR (growth sector region) and wide-GSR, according to the different grain growth directions which are parallel and normal to the rows of seed crystals, respectively. The invading flux measurements revealed that the magnetic flux invades the sample from the wide-GSR prior to the narrow-GSR. It suggests that such anisotropic grain growth leads to different distributions of pinning centers, variations of J c values, and the formation of preferential paths for the invading magnetic fluxes. Using lower applied fields definitely contributed to lowering the heat generation during the PFM process, which, in turn, led to enhanced trapped magnetic fluxes.
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DOI:
10.1088/1742-6596/507/1/012039
发表时间:
2014
期刊:
Journal of Physics: Conference Series
影响因子:
--
作者:
T. Oka;Y. Yamada;T. Horiuchi;J. Ogawa;S. Fukui;T. Sato;K. Yokoyama;M. Langer
通讯作者:
M. Langer
DOI:
10.1088/1742-6596/400/2/022089
发表时间:
2012
期刊:
Journal of Physics: Conference Series
影响因子:
--
作者:
T. Oka;H. Seki;D. Ishiduka;J. Ogawa;S. Fukui;T. Sato;K. Yokoyama;A. Murakami
通讯作者:
A. Murakami
影响因子:
1.7
作者:
T. Oka;D. Ishiduka;J. Ogawa;S. Fukui;Takashi Sato;K. Yokoyama;A. Murakami;H. Stopfel
通讯作者:
H. Stopfel
DOI:
10.1016/j.phpro.2014.09.021
发表时间:
2014
期刊:
Physics Procedia
影响因子:
--
作者:
T. Oka;Y. Yamada;T. Horiuchi;J. Ogawa;S. Fukui;Takashi Sato;K. Yokoyama;M. Langer
通讯作者:
M. Langer
影响因子:
3.6
作者:
Durrell, J. H.;Dennis, A. R.;Cardwell, D. A.
通讯作者:
Cardwell, D. A.