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HHFW heating efficiency on NSTX versus Bφ and antenna k

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

HHFW RF power delivered to the core plasma of NSTX is strongly reduced as the launched wavelength is increased - for B=4.5kG, heating is ∼1/2 as effective at k=-7m-1 as at 14m-1 and ∼1/10 as effective at -3m-1. Measured edge ion heating, attributable to parametric decay (PDI), increases with wavelength but not fast enough to account for the observed power loss. Surface fast waves (FW) may enhance both PDI and also losses in sheaths and structures around the machine - FW fields propagate closer to the wall with decreasing B and k (onset n e∝B×k2). A dramatic increase in core heating efficiency is observed at -7m-1 when B is increased to 5.5 kG - central Te near 4 keV at PRF=2MW. Also, the PDI losses are a weak function of B and k, whereas the far-field RF poloidal magnetic field (at 5.5 kG) increases a factor of ∼3 when k is reduced from 14m-1 to -3m-1, suggesting a large increase in wall/sheath power loss and a major effect of surface fast waves on edge losses.

Original languageEnglish (US)
Title of host publicationRADIO FREQUENCY POWER IN PLASMAS
Subtitle of host publication17th Topical Conference on Radio Frequency Power in Plasmas
Pages107-110
Number of pages4
DOIs
StatePublished - 2007
Event17th Topical Conference on Radio Frequency Power in Plasmas - Clearwater, FL, United States
Duration: May 7 2007May 9 2007

Publication series

NameAIP Conference Proceedings
Volume933
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

Other17th Topical Conference on Radio Frequency Power in Plasmas
Country/TerritoryUnited States
CityClearwater, FL
Period5/7/075/9/07

All Science Journal Classification (ASJC) codes

  • General Physics and Astronomy

Keywords

  • Electron energy and confinement time
  • RF Heating
  • Spherical torus

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