Title
HHFW heating efficiency on NSTX versus Bφ and antenna k ∥
Date Issued
14 December 2007
Access level
metadata only access
Resource Type
conference paper
Author(s)
Hosea J.
Bell R.
Bernabei S.
Leblanc B.
Phillips C.K.
Ryan P.
Sabbagh S.
Tritz K.
Wilgen J.
Wilson J.R.
Yuh H.
Johns Hopkins University
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×k∥2). 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. © 2007 American Institute of Physics.
Start page
107
End page
110
Volume
933
Language
English
OCDE Knowledge area
Electroquímica
Física de partículas, Campos de la Física
Subjects
Scopus EID
2-s2.0-36849076105
ISSN of the container
15517616
ISBN of the container
978-073540444-1
Conference
AIP Conference Proceedings - 17th Topical Conference on Radio Frequency Power in Plasmas
Sources of information:
Directorio de Producción Científica
Scopus