Finding the Optimum Frequency and the H- Distribution in the HERA RF- Volume Ion Source
Description
The HERA RF-Volume Source is the only source available that delivers routinely an H- current of 40 mA without Cs. The dependency of the quality of the H- beam on the frequency was investigated. A frequency range of 1.65 - 9 Mhz was scanned and the emittance was measured for several H- currents up to 40 mA. The production mechanism for H- ions in this type of source is still under discussion. Laser photodetachment measurements have been started at DESY in order to measure the H- distribution in the source. The measurements have also been done under extraction conditions at high voltage. The results of the measurements with and without extraction are a basis for the development of a theory for the transition between plasma and vacuum (sheath), a cornerstone for beam transport programs. Knowledge of the H- distribution and where they are produced makes further source improvements possible
Additional details
Identifiers
- DOI
- 10.1063/1.1908297;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 763
- Journal Issue
- 1
- Journal Page Range
- p. 214-228
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 10. international symposium on production and neutralization of negative ions and beams
- Dates
- 14-17 Sep 2004
- Place
- Kiev (Ukraine)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36073635
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS; S43: PARTICLE ACCELERATORS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANIONS; BEAM TRANSPORT; DESY; DISTRIBUTION; ELECTRIC CURRENTS; HERA STORAGE RING; HYDROGEN IONS; ION BEAMS; ION SOURCES; LASERS; MHZ RANGE; PLASMA; RF SYSTEMS
- Descriptors DEC
- ACCELERATORS; BEAMS; CHARGED PARTICLES; CURRENTS; CYCLIC ACCELERATORS; FREQUENCY RANGE; IONS; STORAGE RINGS; SYNCHROTRONS
Optional Information
- Notes
- (c) 2005 American Institute of Physics