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Progress in the Study of RF Heating and Stabilization on HANBIT Mirror Device

Authors :
D. K. Lee
K. Choh
S. W. Yoon
S. J. Yoo
J. G. Bak
W. H. Ko
M. K. Park
A.C. England
H. G. Lee
T. Lho
J. S. Hong
M. Kwon
J. S. Yoon
J. H. Choi
J. Y. Kim
H. K. Na
J. H. Lee
S. H. Seo
H. G. Jhang
J. W. Choi
J. H. Yeom
S. S. Kim
Dongcheol Seo
K. I. You
B. H. Park
S. G. Lee
Source :
Fusion Science and Technology. 47:17-22
Publication Year :
2005
Publisher :
Informa UK Limited, 2005.

Abstract

The HANBIT device is a simple mirror-type device of which the length, radius, and magnetic field are about 5 m, 0.18 m, and 0.1-0.3 T, respectively, in the central cell. In HANBIT, two antenna systems are used for the plasma production, heating, and MHD stabilization; one is the slot antenna located near the center region with the maximum power of 500 kW and the typical frequency of 3.5 MHz, and the other DHT antenna located near the mirror throat with the maximum power of 100 kW and the frequency of 3.75 MHz. Recent experimental studies in HANBIT indicate that the slot antenna system can produce stable, high-density plasmas in apparently two different regimes; one is the fast wave regime with the ratio w/Wci∼2 and the other is the slow wave regime with w

Details

ISSN :
19437641 and 15361055
Volume :
47
Database :
OpenAIRE
Journal :
Fusion Science and Technology
Accession number :
edsair.doi...........f779d9fb9d589ef2afc864673897f7a6