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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 |
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Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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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. |
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ISSN: | 0921-4534 1873-2143 |
DOI: | 10.1016/j.physc.2004.06.011 |