Published March 10, 2009 | Version v1
Journal article

Optimal Parameters of High Energy Ion Microprobe Systems Comprised of Oxford Lenses

  • 1. Louisiana Accelerator Center/Physics Dept, University of Louisiana at Lafayette, P.O. Box 42410, Lafayette LA 70504-2410 (United States)
  • 2. Instituto de Fisica, UNIVERSIDADE FEDERAL DO RIO GRANDE DO SUL, Av. Bento Goncalves, 9500, C.P. 15051, Porto Alegre Rio Grande do Sul 91501-970 (Brazil)
  • 3. Louisiana Accelerator Center, University of Louisiana at Lafayette, P.O. Box 42410, Lafayette LA 70504-2410 (United States)

Description

Focusing of ion beams of MeV energy until now has been mostly accomplished by magnetic quadrupole lenses in different configurations: doublet, triplet, quadruplet and quintuplet. Many focusing systems are two-parametric focusing systems, i.e., systems having two field parameters (two excitations). The simplest two parametric focusing system, other than the doublet, is a two parametric triplet which can consist of two different configurations: (1) an Oxford configuration in which the focusing (F) and defocusing (D) capabilities of the lenses in one plane alternate F-D-F whereas the lens strengths are ordered as A-A-B, and (2) a triplet in which the focusing and defocusing capabilities of the lenses in one plane also alternate F-D-F but the lens strengths are ordered as A-B-A. Experimental results of a comparison of system parameters for these two focusing configurations, including demagnifications, magnet current, and slit settings will be shown. Both configurations utilized the Oxford Microbeams, Ltd. 10 cm long magnetic quadrupole lenses.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1099
Journal Issue
1
Journal Page Range
p. 292-295
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
12. international conference on application of accelerators in research and industry
Acronym
CAARI 2008
Dates
10-15 Aug 2008
Place
Fort Worth, TX (United States)

INIS

Optional Information

Notes
(c) 2009 American Institute of Physics