DocumentCode
868757
Title
Aperture Limits Due to the Presence of Higher Magnetic Field Multipoles
Author
Parzen, G.
Author_Institution
Brookhaven National Laboratory Upton, New York 11973
Volume
30
Issue
4
fYear
1983
Firstpage
2421
Lastpage
2423
Abstract
Superconducting magnets tend to produce magnetic fields which have larger higher systematic multipoles and larger random multipoles than conventional magnets. The current carrying coils in superconducting magnets are usually not shielded by the iron yoke, and thus the magnetic field shape is determined by the current distribution rather than the shape of an iron surface. Higher systematic magnetic field multipoles are then generated by necessary deviations of the current distribution from the ideal desired distribution; random multipoles are generated by errors in the location of the current carrying conductors. The presence of these undesired field multipoles will limit the good field aperture of the accelerator. One effect of these multipoles is that they will distort the working line, the dependencies of the ¿-values, ¿X ¿y, on the momentum ¿p/p. Another effect of these multipoles is to produce linear and non-linear stop bands. This paper is concerned primarily with aperture limits due to the distortion of the working line. Distortion of the working line produced by the lower field multipoles is usually corrected with a correction coil system provided for that purpose. The working line distortion that remains is that due to higher field multipoles that cannot be corrected with the correction coil system. The magnetic field due to the higher multipoles vary like some high power of r, the radial distance from the magnet center, like at least r6 in the case of the CBA (Colliding Beam Accelerator at BNL).
Keywords
Apertures; Conductors; Current distribution; Iron; Magnetic fields; Magnetic shielding; Nonlinear distortion; Shape; Superconducting coils; Superconducting magnets;
fLanguage
English
Journal_Title
Nuclear Science, IEEE Transactions on
Publisher
ieee
ISSN
0018-9499
Type
jour
DOI
10.1109/TNS.1983.4332834
Filename
4332834
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