Abstract
We present novel experimental evidence of parametric decay instability of microwave beams in the plasma edge of the Wendelstein 7-X stellarator. We propose that the instability is sustained by trapping of only one daughter wave in the non-monotonic density profile measured with high spatial resolution within a stationary magnetic island. The power levels and spectral shapes of the detected microwave signal are reproduced by numerical modelling and a theoretical power threshold is predicted around 300 kW, comparable with observations. We predict a fraction of power drained by daughter waves around 4% in the experiments, potentially increasing above 50% for more hollow edge density profiles. Such absorption levels could significantly reduce the efficiency of the microwave heating and current-drive system in tokamaks and stellarators.
Original language | English |
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Article number | 074003 |
Journal | Nuclear Fusion |
Volume | 62 |
Issue number | 7 |
Number of pages | 6 |
ISSN | 0029-5515 |
DOIs | |
Publication status | Published - 2022 |
Keywords
- Collective Thomson scattering
- Electron cyclotron resonance heating
- Ion Bernstein waves
- Parametric decay instability
- Upper hybrid wave
- Wendelstein 7-X stellarator