Sep 20 – 25, 2026
Prestige Lakeside Resort Nelson
America/Vancouver timezone
Registration and Abstract submission is OPEN

Ion Source Development for AMS at WHOI

Sep 21, 2026, 2:25 PM
25m
Conference Room (Prestige Lakeside Resort Nelson)

Conference Room

Prestige Lakeside Resort Nelson

Speaker

Dr Mark Roberts (Woods Hole Oceanographic Institution)

Description

Accelerator mass spectrometry (AMS) is a sensitive technique for counting single atoms. The technique was developed in nuclear physics laboratories in the late 1970s for $^{14}$C, and subsequently extended to other isotopes, including $^{10}$Be, $^{36}$Cl, and $^{129}$I. In general, the AMS method employs a positive high-voltage tandem accelerator to accelerate negative ions. Almost exclusively, the negative ions are produced by cesium sputtering sources. Cesium sputter sources have a long history, much of it intimately linked to the development of AMS. Despite nearly five decades of development, the ion source remains the most maintenance-intensive and least understood component of an AMS system. We present some of our efforts to improve the performance of our cesium sputtering source, and additionally, our experience with a novel gas-accepting ECR-type ion source coupled to a charge exchange canal.

Email address mroberts@whoi.edu
Funding Agency United States National Science Foundation under Cooperative Agreement OCE-2244731
Classification Applications of Negative sources - medical (diagnostics, therapy), industrial (implantation, materials analysis, carbon dating, discovery science

Author

Dr Mark Roberts (Woods Hole Oceanographic Institution)

Co-author

Dr Joshua D. Hlavenka (Argonne National Laboratory)

Presentation materials

There are no materials yet.