Improved operation of the nonambipolar electron source
Creators
- 1. University of Wisconsin-Madison, Madison, Wisconsin 53706 (United States)
Description
Significant improvements have been made to the nonambipolar electron source (NES), a radio frequency (rf) plasma-based electron source that does not rely on electron emission at a cathode surface [B. Longmier, S. Baalrud, and N. Hershkowitz, Rev. Sci. Instrum. 77, 113504 (2006)]. A prototype NES has produced 30 A of continuous electron current, using 2 SCCM (SCCM denotes cubic centimeter per minute at STP) Xe, 1300 W rf power at 13.56 MHz, yielding a 180 times gas utilization factor. A helicon mode transition has also been identified during NES operation with an argon propellant, using 15 SCCM Ar, 1000 W rf, and 100 G magnetic field. This NES technology has the ability to replace hollow cathode electron sources and to enable high power electric propulsion missions, eliminating one of the lifetime restrictions that many ion thrusters have previously been faced with.
Additional details
Identifiers
- DOI
- 10.1063/1.2979012;
Publishing Information
- Journal Title
- Review of Scientific Instruments
- Journal Volume
- 79
- Journal Issue
- 9
- Journal Page Range
- p. 093506-093506.8
- ISSN
- 0034-6748
- CODEN
- RSINAK
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41015915
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S43: PARTICLE ACCELERATORS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ARGON; CURRENTS; ELECTRON EMISSION; ELECTRON SOURCES; ELECTRONS; HOLLOW CATHODES; ION THRUSTERS; LIFETIME; MAGNETIC FIELDS; MHZ RANGE 01-100; OPERATION; PLASMA; PROPULSION; RADIOWAVE RADIATION
- Descriptors DEC
- CATHODES; ELECTRODES; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ELEMENTS; EMISSION; FERMIONS; FLUIDS; FREQUENCY RANGE; GASES; LEPTONS; MHZ RANGE; NONMETALS; PARTICLE SOURCES; RADIATION SOURCES; RADIATIONS; RARE GASES; THRUSTERS
Optional Information
- Notes
- (c) 2008 American Institute of Physics