Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Microwave imaging reflectometry studies for turbulence diagnostics on KSTAR

Journal Article · · Review of Scientific Instruments
DOI:https://doi.org/10.1063/1.3499606· OSTI ID:22055832
; ; ; ; ;  [1]; ; ;  [2];  [3]
  1. Pohang University of Science and Technology, Pohang, Gyeongbuk 790-784 (Korea, Republic of)
  2. University of California at Davis, Davis, California 95616 (United States)
  3. Kyungbuk University, Gyeongbuk 702-701 (Korea, Republic of)
The first prototype microwave imaging reflectometry (MIR) system [H. Park et al., Rev. Sci. Instrum. 74, 4239 (2004)] clearly demonstrated the shortcomings of conventional reflectometry when the probe beam encountered a large amplitude and/or high fluctuation wavenumber at the reflection layer in laboratory tests, the distinctive advantages shown in these tests were not fully realized in the plasma operation. To understand the discrepancies, the MIR system performance has been thoroughly investigated at POSTECH. In this paper, a possible cause of the MIR performance degradation on TEXTOR will be presented together with a concept of multifrequency MIR system design that will be developed for KSTAR.
OSTI ID:
22055832
Journal Information:
Review of Scientific Instruments, Journal Name: Review of Scientific Instruments Journal Issue: 10 Vol. 81; ISSN 0034-6748; ISSN RSINAK
Country of Publication:
United States
Language:
English

Similar Records

A synthetic diagnostic for the evaluation of new microwave imaging reflectometry diagnostics for DIII-D and KSTAR
Journal Article · Fri Oct 15 00:00:00 EDT 2010 · Review of Scientific Instruments · OSTI ID:22055814

Comparative study between the reflective optics and lens based system for microwave imaging system on KSTAR
Journal Article · Fri Oct 15 00:00:00 EDT 2010 · Review of Scientific Instruments · OSTI ID:22058706

Effects of asymmetry and target location on microwave imaging reflectometry
Journal Article · Fri Oct 01 00:00:00 EDT 2004 · Review of Scientific Instruments · OSTI ID:20636757