Paper | Title | Page |
---|---|---|
MOXZO01 | Status of the 45 GHz MARS-D ECRIS | 17 |
|
||
Funding: This work was supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under contract number DE-AC02-05CH11231 Development of the MARS-D ECR ion source, a 45 GHz next generation ECRIS using a NbTi MARS-magnet, has been continuously moving forward at LBNL. Recent stress analyses and other key components of the MARS-D ion source have been essentially finalized. This article presents and discusses the status of this new 45 GHz ECR ion source, such as the latest design features and the fabrication plan with funding available in the very near future. |
||
Slides MOXZO01 [3.661 MB] | ||
DOI • | reference for this paper ※ https://doi.org/10.18429/JACoW-ECRIS2020-MOXZO01 | |
About • | Received ※ 25 September 2020 — Revised ※ 02 October 2020 — Accepted ※ 01 December 2020 — Issue date ※ 29 November 2021 | |
Cite • | reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml) | |
TUXZO01 | A Proposed Explanation of High-Minimum-B Instabilities | 68 |
|
||
It is well-known that electron cyclotron resonance ion sources exhibit instabilities when these sources’ minimum magnetic fields are approximately 80% of the resonant field or greater, but the reasons for this instability have yet to be satisfactorily explained. We show that raising the minimum field makes much faster heating modes accessible at lower energies that invite the onset of kinetic instabilities. | ||
Slides TUXZO01 [3.566 MB] | ||
DOI • | reference for this paper ※ https://doi.org/10.18429/JACoW-ECRIS2020-TUXZO01 | |
About • | Received ※ 28 September 2020 — Revised ※ 06 October 2020 — Accepted ※ 03 December 2020 — Issue date ※ 13 December 2020 | |
Cite • | reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml) | |