journals.iop.org home page electronic journals * User guide   * Site map   | Quick Search:Help  
Superconductor Science and Technology
Athens/Institutional login
IOP login: Password:   
Create account | Alerts | Contact us
Journals Home | Journals List | EJs Extra | This Journal | Search | Authors | Referees | Librarians | User Options | Help |

Pulsed-field magnetization of drilled bulk high-temperature superconductors: flux front propagation in the volume and on the surface

Gregory P Lousberg et al 2009 Supercond. Sci. Technol. 22 125026 (9pp)   doi: 10.1088/0953-2048/22/12/125026  Help

   PDF (877 KB) | References

Gregory P Lousberg1,2, J-F Fagnard1, E Haanappel3,4, X Chaud5, M Ausloos6, B Vanderheyden1 and Ph Vanderbemden1
1 SUPRATECS Research Group, Department of Electrical Engineering and Computer Science (B28), University of Liège, Belgium
2 Laboratoire National des Champs Magnétiques Intenses (LNCMI), Toulouse, France
3 IPBS-UPS/CNRS UMR5089, Toulouse, France
4 UPS, IPBS, Université de Toulouse, Toulouse, France
5 CNRS, CRETA, Grenoble, France
6 SUPRATECS (B5a), University of Liège, Belgium
E-mail: gregory.lousberg@ulg.ac.be

Abstract. We present a method for characterizing the propagation of the magnetic flux in an artificially drilled bulk high-temperature superconductor (HTS) during pulsed-field magnetization. As the magnetic pulse penetrates the cylindrical sample, the magnetic flux density is measured simultaneously in 16 holes by means of microcoils that are placed across the median plane, i.e. at an equal distance from the top and bottom surfaces, and close to the surface of the sample. We discuss the time evolution of the magnetic flux density in the holes during a pulse and measure the time taken by the external magnetic flux to reach each hole. Our data show that the flux front moves faster in the median plane than on the surface when penetrating the sample edge; it then proceeds faster along the surface than in the bulk as it penetrates the sample further. Once the pulse is over, the trapped flux density inside the central hole is found to be about twice as large in the median plane as on the surface. This ratio is confirmed by modelling.

Print publication: Issue 12 (December 2009)
Received 13 August 2009, in final form 21 September 2009
Published 23 October 2009

Bookmark and Share Post to CiteUlike | Post to Connotea | Post to Bibsonomy

 

Find related articles





Article options

Authors & Referees

IOP Journal Archiveauthor services
 
Content finder
  Full Search
  Help


  
Setup information is available for Adobe Acrobat.
EndNote, ProCite ® and Reference Manager ® are registered trademarks of ISI Researchsoft.
Copyright © Institute of Physics and IOP Publishing Limited 2009.
Use of this service is subject to compliance with the Terms and Conditions of use. In particular, reselling and systematic downloading of files is prohibited.
Help: Cookies | Data Protection. Privacy policy Disclaimer