Abstract

The magnetization and low field stability were measured on a series of high current-density Nb <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> Sn strands with 54 to 198 sub-elements taken from accelerator magnet development programs. The effective filament size, <i xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">d<sub>eff</sub> </i> ,, as determined from the width of the magnetization loop at low field and the extrapolation of the transport critical current from high field, was very close to the sub-element diameter determined by the strand geometry. Self-field corrections were vital for obtaining this agreement; without them, <i xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">d<sub>eff</sub> </i> was overestimated by ~25%. While all strands, even those with <i xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">d<sub>eff</sub> </i> as small as 35 mum, exhibited flux-jumps at low field in magnetization measurements, smaller sub-elements produced smaller flux-jump magnitude and a smaller range of field over which flux jumps occurred, suggesting stability improved with decreasing <i xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">d<sub>eff.</sub> </i> . However, good combinations of the residual resistivity ratio <i xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">RRR</i> and the critical current density became increasingly difficult to obtain by varying the reaction heat treatment as the sub-element number increased. Further analyses of <i xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">RRR </i> data indicate that tin contamination of the copper stabilizer is underway even before any Nb <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">3</sub> Sn is formed in strands with high numbers of sub-elements.

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