Abstract
We apply the continuous wavelet transform (CWT) and a CWT spectral technique to the analysis of the time-resolved fluctuation-driven particle flux in the H-1 heliac. The results confirm that in some cases the outward radial flux reverses its direction. In addition, time-resolved frequency spectra of fluctuation signals obtained by CWT show that the dominant frequency component as a function of time closely follows changes in the radial electric field. This suggests that the VEXB drift velocity dominates the poloidal phase velocity of the fluctuations in the laboratory frame, in which case the time-resolved frequency can be used to characterize the radial electric field.
Original language | English |
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Pages (from-to) | 503-505 |
Number of pages | 3 |
Journal | Review of Scientific Instruments |
Volume | 72 |
Issue number | 1 |
DOIs | |
Publication status | Published - Jan 2001 |