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Featured researches published by Roger D. Dwinell.


Review of Scientific Instruments | 2004

Results with the superconducting electron cyclotron resonance ion source VENUS (invited)

Claude M. Lyneis; Daniela Leitner; Steve R. Abbott; Roger D. Dwinell; M. Leitner; C. S. Silver; C. Taylor

During the last year, the VENUS electron cyclotron resonance (ECR) ion source was commissioned at 18 GHz and preparations for 28 GHz operation, which is set to begin early in 2004, are now underway. The goal of the VENUS ECR ion source project as the RIA research and development injector is the production of 240 eμA of U30+, a high current medium charge state beam. On the other hand, as an injector ion source for the 88-Inch Cyclotron the design objective is the production of 5 eμA of U48+, a low current, very high charge state beam. During the commissioning phase with 18 GHz, tests with various gases and recently metals have been performed with up to 2000 W rf power and the performance is very promising. For example, 1100 eμA of O6+, 180 eμA of Ar12+, 150 eμA of Xe20+, and 100 eμA of Bi24+ were produced in the early commissioning phase, ranking VENUS among the currently highest performance 18 GHz ECR ion sources. The emittance of the beams produced at 18 GHz was measured with a two axis emittance scanner...


ELECTRON CYCLOTRON RESONANCE ION SOURCES: 16th International Workshop on ECR Ion Sources ECRIS'04 | 2005

First Results of the Superconducting ECR Ion Source Venus with 28 GHz

Daniela Leitner; Claude M. Lyneis; Steve R. Abbott; Roger D. Dwinell; D. Collins; M. Leitner

VENUS (Versatile ECR ion source for NUclear Science) is a next generation superconducting ECR ion source, designed to produce high current, high charge state ions for the 88‐Inch Cyclotron at the Lawrence Berkeley National Laboratory. VENUS also serves as the prototype ion source for the RIA (Rare Isotope Accelerator) front end. The magnetic confinement configuration consists of three superconducting axial coils and six superconducting radial coils in a sextupole configuration. The nominal design fields of the axial magnets are 4T at injection and 3T at extraction; the nominal radial design field strength at the plasma chamber wall is 2T, making VENUS the world most powerful ECR plasma confinement structure. From the beginning, VENUS has been designed for optimum operation at 28 GHz with high power (10 kW).In 2003 the VENUS ECR ion source was commissioned at 18 GHz, while preparations for 28 GHz operation were being conducted. During this commissioning phase with 18 GHz, tests with various gases and metal...


Proceedings of the 2003 Particle Accelerator Conference | 2003

Commissioning of the superconducting ECR ion source VENUS

Daniela Leitner; Steve R. Abbott; Roger D. Dwinell; M. Leitner; C. Taylor; Claude M. Lyneis

VENUS (Versatile ECR ion source for NUclear Science) is a next generation superconducting ECR ion source, designed to produce high current, high charge state ions for the 88-Inch Cyclotron at the Lawrence Berkeley National Laboratory. VENUS also serves as the prototype ion source for the RIA (Rare Isotope Accelerator) front end. The magnetic confinement configuration consists of three superconducting axial coils and six superconducting radial coils in a sextupole configuration. The nominal design fields of the axial magnets are 4T at injection and 3T at extraction; the nominal radial design field strength at the plasma chamber wall is 2T, making VENUS the world most powerful ECR plasma confinement structure. The magnetic field strength has been designed for optimum operation at 28 GHz. The four-year VENUS project has recently achieved two major milestones: The first plasma was ignited in June, the first mass-analyzed high charge state ion beam was extracted in September of 2002. The paper describes the ongoing commissioning. Initial results including first emittance measurements are presented.


Nuclear Instruments & Methods in Physics Research Section B-beam Interactions With Materials and Atoms | 2005

Next generation ECR ion sources: First results of the superconducting 28 GHz ECRIS – VENUS

Daniela Leitner; Claude M. Lyneis; Steve R. Abbott; D. Collins; Roger D. Dwinell; M.L. Galloway; M. Leitner; D. S. Todd


Lawrence Berkeley National Laboratory | 2004

New Results with the superconducting ECR ion source VENUS

Claude M. Lyneis; Daniela Leitner; Steve R. Abbott; Roger D. Dwinell; M. Leitner; C.S. Silver; C. Taylor


Other Information: PBD: 1 Jun 2004 | 2004

Commissioning of the superconducting ECR ion source VENUS at 18 GHz

Daniela Leitner; Steven R. Abbott; Roger D. Dwinell; M. Leitner; Clyde Taylor; Claude M. Lyneis


Archive | 2004

28 GHz operation of the superconducting ECR ion source VENUS

Daniela Leitner; Claude M. Lyneis; Steven R. Abbott; Roger D. Dwinell; D. Collins; Mattheaus Leitner


Lawrence Berkeley National Laboratory | 2004

Development of ECR ion source and LEBT technology for RIA

Daniela Leitner; Claude M. Lyneis; Steven R. Abbott; Roger D. Dwinell; M. Leitner; Charles S. Silver; Clyde Taylor


Archive | 2003

NEW RESULTS WITH VENUS

Claude M. Lyneis; Daniela Leitner; Steve R. Abbott; Roger D. Dwinell; M. Leitner; C.S. Silver; C. Taylor

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Dive into the Roger D. Dwinell's collaboration.

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Claude M. Lyneis

Lawrence Berkeley National Laboratory

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M. Leitner

Lawrence Berkeley National Laboratory

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Steve R. Abbott

Lawrence Berkeley National Laboratory

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C. Taylor

Lawrence Berkeley National Laboratory

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Steven R. Abbott

Lawrence Berkeley National Laboratory

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Clyde Taylor

University of California

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D. Collins

Lawrence Berkeley National Laboratory

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C. S. Silver

Lawrence Berkeley National Laboratory

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Charles S. Silver

Lawrence Berkeley National Laboratory

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