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Shell-Based Support Structure for the 45 GHz ECR Ion Source MARS-D

Journal Article · · IEEE Transactions on Applied Superconductivity
Superconducting electron cyclotron resonance ion sources (ECRISs) using NbTi coils and optimized for 28 GHz resonant heating have been successfully operated for almost two decades. Moving to higher heating frequencies requires increased magnetic fields, but traditional racetrack-and-solenoid ECRIS structures are at their limit using NbTi. Rather than moving to a superconductor untested in this field, we report the Mixed Axial and Radial field System (MARS) being developed at Lawrence Berkeley National Laboratory employs a novel closed-loop-coil design that more efficiently utilizes conductor fields and will allow the use of NbTi in a next-generation, 45 GHz ECRIS. This article presents the design of the shell-based support structure central to the MARS-D magnet design, as well as structural analysis of its components and optimization of pre-load parameters that will guarantee its successful operation.
Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Basic Energy Sciences (BES); USDOE Office of Science (SC), Nuclear Physics (NP)
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1896481
Journal Information:
IEEE Transactions on Applied Superconductivity, Journal Name: IEEE Transactions on Applied Superconductivity Journal Issue: 6 Vol. 32; ISSN 1051-8223
Publisher:
IEEECopyright Statement
Country of Publication:
United States
Language:
English

References (5)

Advanced superconducting electron cyclotron resonance ion source SECRAL: Design, construction, and the first test result journal March 2006
Magnet system for an ECR ion source journal March 2000
Design of a New Superconducting Magnet System for High Strength Minimum-B Fields for ECRIS journal June 2016
Mechanical Study of a Superconducting 28-GHz Ion Source Magnet for FRIB journal August 2019
Superconducting Magnet Development for the HIAF Accelerator Complex journal September 2022

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