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Huge compact flux avalanches in superconducting Nb thin films

Using a magneto-optical technique we perform a quantitative analysis of magnetic flux penetration in superconducting niobium thin films on A-plane ( 1 1 2 ¯ 0 ) sapphire substrates as a function of temperature (1.5 K ⩽ T ⩽ T c = 9.2 K). In these samples we observe huge compact avalanches (HCAs for b...

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Published in:Physica. C, Superconductivity Superconductivity, 2004-09, Vol.411 (1), p.11-17
Main Authors: Welling, M.S., Westerwaal, R.J., Lohstroh, W., Wijngaarden, R.J.
Format: Article
Language:English
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Summary:Using a magneto-optical technique we perform a quantitative analysis of magnetic flux penetration in superconducting niobium thin films on A-plane ( 1 1 2 ¯ 0 ) sapphire substrates as a function of temperature (1.5 K ⩽ T ⩽ T c = 9.2 K). In these samples we observe huge compact avalanches (HCAs for brevity), very much like some snow-avalanches and unlike the rough dendritic flux penetration observed on R-plane ( 1 1 ¯ 0 2 ) sapphire. The behavior observed is consistent with the occurrence of thermo-magnetic avalanches as proposed by Aranson et al. [Phys. Rev. Lett. 87 (2001) 067003]. For increasing temperature, we find: (1) an increased branching of the HCA. (2) An increased applied field necessary for the first HCA to occur. (3) A decrease in the number of HCAs, accompanied by more ‘regular’ flux penetration (above 6.2 K avalanches are completely absent). (4) An increase of the total amount of flux as well as the area of the HCA.
ISSN:0921-4534
1873-2143
DOI:10.1016/j.physc.2004.06.011