DocumentCode
1097386
Title
Design of a
Magnet for a 4th Generation ECR Ion Source
Author
Prestemon, S. ; Trillaud, F. ; Caspi, S. ; Ferracin, P. ; Sabbi, G.L. ; Lyneis, C.M. ; Leitner, D. ; Todd, D.S. ; Hafalia, R.
Author_Institution
Lawrence Berkeley Nat. Lab., Berkeley, CA, USA
Volume
19
Issue
3
fYear
2009
fDate
6/1/2009 12:00:00 AM
Firstpage
1336
Lastpage
1339
Abstract
The next generation of Electron Cyclotron Resonant (ECR) ion sources are expected to operate at a heating radio frequency greater than 40 GHz. The existing 3rd generation systems, exemplified by the state of the art system VENUS, operate in the 10-28 GHz range, and use NbTi superconductors for the confinement coils. The magnetic field needed to confine the plasma scales with the rf frequency, resulting in peak fields on the magnets of the 4th generation system in excess of 10 T. High field superconductors such as Nb3Sn must therefore be considered. The magnetic design of a 4th. generation ECR ion source operating at an rf frequency of 56 GHz is considered. The analysis considers both internal and external sextupole configurations, assuming commercially available Nb3Sn material properties. Preliminary structural design issues are discussed based on the forces and margins associated with the coils in the different configurations, leading to quantitative data for the determination of a final magnet design.
Keywords
accelerator RF systems; accelerator magnets; cyclotron resonance; ion accelerators; ion sources; niobium alloys; plasma accelerators; plasma confinement; plasma sources; superconducting coils; superconducting magnets; tin alloys; ECR ion source; Nb3Sn; VENUS; confinement coils; electron cyclotron resonant generation; frequency 10 GHz to 28 GHz; frequency 56 GHz; heating radio frequency; high-field accelerator magnets; magnet design; magnetic field; plasma scales; superconductor magnet; ${rm Nb}_{3}{rm Sn}$ superconducting magnets; ECR ion source;
fLanguage
English
Journal_Title
Applied Superconductivity, IEEE Transactions on
Publisher
ieee
ISSN
1051-8223
Type
jour
DOI
10.1109/TASC.2009.2017719
Filename
5109527
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