27 September 2026 to 1 October 2026
Hilton San Francisco - Financial District
America/Los_Angeles timezone

Observation of Non-Synchronized Afterglow Pulses and Beam Characterization on SEISM

29 Sept 2026, 16:00
2h
Hilton San Francisco - Financial District

Hilton San Francisco - Financial District

750 Kearny Street, San Francisco, CA 94108
Poster Presentation Poster session

Speaker

Thomas Andre (Laboratoire de Physique Subatomique et de Cosmologie)

Description

SEISM (Sixty-gigahertz Ion Source using Megawatt magnets) is a 60 GHz electron-cyclotron-resonance ion source that achieved in 2014 a record pulsed multicharged-ion current density of about 1 A/cm$^{2}$. Operation resumed in 2021 after upgrades to the beam line, and several experimental campaigns were performed to reproduce the conditions that previously enabled such high extracted currents.

Following the failure of the 60 GHz gyrotron in 2024, the setup was adapted to operate at 18 GHz with a new aluminum plasma chamber manufactured by additive techniques. This new microwave system, capable of both CW and pulsed operation, enabled renewed investigations of SEISM plasmas as well as emittance measurements using a pepperpot diagnostic.

Recent measurements revealed the presence of non-synchronized afterglow pulses, so far observed exclusively on SEISM. Although still under investigation, this phenomenon appears promising for advancing our understanding of CUSP-based plasma physics. Emittance scans have also identified distinct charge-state populations in argon plasmas and quantified the influence of microwave pulse duration and bias-disk voltage on beam quality and extracted current. These recent developments and results will be presented.

Classification MC1: New developments and status reports
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Author

Thomas Andre (Laboratoire de Physique Subatomique et de Cosmologie)

Co-authors

Andrea Cernuschi (Laboratoire de Physique Subatomique et de Cosmologie) Christophe Peaucelle (Laboratoire de Physique Subatomique et de Cosmologie) Mr Etienne Labussiere (Laboratoire de Physique Subatomique et de Cosmologie) François Debray (Centre National de la Recherche Scientifique) Julien Angot (Laboratoire de Physique Subatomique et de Cosmologie) Maud Baylac (Laboratoire de Physique Subatomique et de Cosmologie) Mr Patrick Sole (Laboratoire de Physique Subatomique et de Cosmologie) Mr Pierre-Olivier Dumont (Laboratoire de Physique Subatomique et de Cosmologie) Mr Quentin Hars (Laboratoire de Physique Subatomique et de Cosmologie) Thomas Thuillier (Lawrence Berkeley National Laboratory)

Presentation materials

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