Interpretation of neutral beam emission spectra as the beam-component density distribution
- 1. Plasma Science and Fusion Center, MIT, Cambridge, Massachusetts (United States)
- 2. Fusion Research Center, The University of Texas at Austin, Austin, Texas (United States)
Description
Diagnostic neutral beams (DNBs) are used on tokamaks and stellarators for measurement of ion temperature, plasma current density, and other critical quantities. It is important to optimize the density in the energy components of the DNB for the diagnostic application. Measured component densities are also useful for interpretation of beam diagnostics and for design of new diagnostics. The spectrally resolved photon emission from the interaction of the neutral beam with a background neutral gas is commonly used for this measurement. The emission cross sections available for interpretation of the measurement are reviewed here. Simulations employ these cross sections with other data to infer the properties of the plasma sources from which the beams are extracted. The simulations are also reviewed. Empirical examples are drawn from beam emission spectra measured for beams installed at the Alcator C-Mod facility
Additional details
Identifiers
- DOI
- 10.1063/1.1784511;
Publishing Information
- Journal Title
- Review of Scientific Instruments
- Journal Volume
- 75
- Journal Issue
- 10
- Journal Page Range
- p. 3487-3489
- ISSN
- 0034-6748
- CODEN
- RSINAK
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36079994
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ALCATOR DEVICE; CROSS SECTIONS; DEPARTURE NUCLEATE BOILING; ELECTRON TEMPERATURE; EMISSION SPECTRA; ION TEMPERATURE; PHOTON EMISSION; PLASMA DENSITY; PLASMA DIAGNOSTICS; PLASMA SIMULATION; STELLARATORS
- Descriptors DEC
- BOILING; CLOSED PLASMA DEVICES; EMISSION; NUCLEATE BOILING; PHASE TRANSFORMATIONS; SIMULATION; SPECTRA; THERMONUCLEAR DEVICES; TOKAMAK DEVICES
Optional Information
- Notes
- (c) 2004 American Institute of Physics