Improved common-path fast-scanning heterodyne interferometer system as potential dense-plasma diagnostics
Creators
- 1. Department of Nuclear Engineering, Seoul National University, Seoul 151-742 (Korea, Republic of)
Description
An improved common-path fast-scanning heterodyne interferometer system has been developed. The mechanical vibration is one of the most critical error sources in typical interferometry system. These errors can be mostly eliminated in a common-path interferometry using a full common-mode rejection scheme. Taking advantage of it, the common-path interferometry is suitable for the measurements in noisy environments and can be applied even to the scanning interferometry. A prototype common-path interferometer system with He-Ne laser has been constructed with the capability of fast scanning by adding a rotating polygon mirror. A test of this system has been completed successfully by measuring the thickness profile of the scratched glass. In this study, the interferometer system is proposed and discussed as a potential density profile diagnostics for dense plasmas. By using a CO2 laser instead of a He-Ne laser, it may also be applied to get the time evolution of steep density profiles of plasma transport barriers in tokamak plasmas
Additional details
Identifiers
- DOI
- 10.1063/1.1786639;
Publishing Information
- Journal Title
- Review of Scientific Instruments
- Journal Volume
- 75
- Journal Issue
- 10
- Journal Page Range
- p. 3417-3419
- ISSN
- 0034-6748
- CODEN
- RSINAK
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36079973
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- CARBON DIOXIDE LASERS; ERRORS; GLASS; INTERFEROMETERS; INTERFEROMETRY; PLASMA DENSITY; PLASMA DIAGNOSTICS; REFRACTIVE INDEX; TOKAMAK DEVICES
- Descriptors DEC
- CLOSED PLASMA DEVICES; GAS LASERS; LASERS; MEASURING INSTRUMENTS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; THERMONUCLEAR DEVICES
Optional Information
- Notes
- (c) 2004 American Institute of Physics