Published April 6, 2005 | Version v1
Journal article

Finding the Optimum Frequency and the H- Distribution in the HERA RF- Volume Ion Source

Creators

  • 1. DESY, Hamburg (Germany)

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

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