Abstract:Isotope effects of ECRH plasma in LHD were investigated in detail. A clear difference of transport and turbulence characteristics in H and D plasmas was found in the core region, with normalized radius <0.8 in high collisionality regime. On the other hand, differences of transport and turbulence were relatively small in low collisionality regime. Power balance analysis and neoclassical calculation showed a reduction of the anomalous contribution to electron and ion transport in D plasma compared with H plasma… Show more
“…This might be an effect of changes in the plasma profiles, in particular of the peaking of n e in the edge, by the combined effect of the extra electron source provided by the injected powder and the real-time reduction of recycling, finally resulting in a more hollow profile in the centre of the plasma. Hollow density profiles have been reported to increase the stability of ion temperature gradient modes in the LHD, reducing turbulence fluctuations 22,28 . Another possibility is turbulence being reduced by The experimental τ E is plotted against the predicted energy confinement time from the international stellarator scaling T E,ISS04 (ref.…”
Section: Discussionmentioning
confidence: 99%
“…In refs. 21,22 , similar phase-contrast imaging measurements were compared with gyrokinetic simulations, determining that the observed fluctuations are indeed due to ion temperature-gradient turbulence. Dedicated gyrokinetic simulations are needed to confirm this result for the cases discussed here and are planned for future work.…”
Section: Performance Improvement and Turbulence Suppressionmentioning
In state-of-the-art stellarators, turbulence is a major cause of the degradation of plasma confinement. To maximize confinement, which eventually determines the amount of nuclear fusion reactions, turbulent transport needs to be reduced. Here we report the observation of a confinement regime in a stellarator plasma that is characterized by increased confinement and reduced turbulent fluctuations. The transition to this regime is driven by the injection of submillimetric boron powder grains into the plasma. With the line-averaged electron density being kept constant, we observe a substantial increase of stored energy and electron and ion temperatures. At the same time, the amplitude of the plasma turbulent fluctuations is halved. While lower frequency fluctuations are damped, higher frequency modes in the range between 100 and 200 kHz are excited. We have observed this regime for different heating schemes, namely with both electron and ion cyclotron resonant radio frequencies and neutral beams, for both directions of the magnetic field and both hydrogen and deuterium plasmas.
“…This might be an effect of changes in the plasma profiles, in particular of the peaking of n e in the edge, by the combined effect of the extra electron source provided by the injected powder and the real-time reduction of recycling, finally resulting in a more hollow profile in the centre of the plasma. Hollow density profiles have been reported to increase the stability of ion temperature gradient modes in the LHD, reducing turbulence fluctuations 22,28 . Another possibility is turbulence being reduced by The experimental τ E is plotted against the predicted energy confinement time from the international stellarator scaling T E,ISS04 (ref.…”
Section: Discussionmentioning
confidence: 99%
“…In refs. 21,22 , similar phase-contrast imaging measurements were compared with gyrokinetic simulations, determining that the observed fluctuations are indeed due to ion temperature-gradient turbulence. Dedicated gyrokinetic simulations are needed to confirm this result for the cases discussed here and are planned for future work.…”
Section: Performance Improvement and Turbulence Suppressionmentioning
In state-of-the-art stellarators, turbulence is a major cause of the degradation of plasma confinement. To maximize confinement, which eventually determines the amount of nuclear fusion reactions, turbulent transport needs to be reduced. Here we report the observation of a confinement regime in a stellarator plasma that is characterized by increased confinement and reduced turbulent fluctuations. The transition to this regime is driven by the injection of submillimetric boron powder grains into the plasma. With the line-averaged electron density being kept constant, we observe a substantial increase of stored energy and electron and ion temperatures. At the same time, the amplitude of the plasma turbulent fluctuations is halved. While lower frequency fluctuations are damped, higher frequency modes in the range between 100 and 200 kHz are excited. We have observed this regime for different heating schemes, namely with both electron and ion cyclotron resonant radio frequencies and neutral beams, for both directions of the magnetic field and both hydrogen and deuterium plasmas.
“…In Refs. [17,18], similar PCI measurements were compared with gyrokinetic simulations, determining that the observed fluctuations are indeed due to ITG turbulence. Dedicated gyrokinetic simulations are needed to confirm this result for the cases exposed here, and are foreseen for future works.…”
Section: Resultsmentioning
confidence: 99%
“…plasma quantities, in particular of the peaking of n e in the edge, resulting in a more hollow profile in the center of the plasma. Hollow density profiles have been reported to increase ITG stability, reducing turbulence fluctuations [18,21]. Another possibility is turbulence being reduced by the increased effective charge Z ef f due to B injection, also referred to as plasma dilution.…”
We report the first observation of a novel confinement regime in a stellarator plasma, characterized by increased confinement and reduced turbulent fluctuations. The transition to this new regime is driven by the injection of sub-millimetric boron powder grains into the plasma. With the line averaged electron density being kept constant, substantial increase of stored energy, electron and ion temperature have been observed. At the same time, the amplitude of the plasma turbulent fluctuations is halved. While lower frequency fluctuations are damped, higher frequency modes in the range 100 ≤ f [kHz] ≤ 200 are excited. The access to this regime has been observed for different heating schemes, namely with both electron and ion cyclotron resonant radio frequency, and neutral beams, for both directions of the magnetic field, and for both hydrogen and deuterium plasmas.
“…18 The ion scale turbulence observations have been compared with the gyrokinetic simulation (GKV 19,20 ) results. [21][22][23] The introduction of this electron scale turbulence measurement will allow for a more detailed comparative study.…”
A 90 GHz W-band millimeter-wave back-scattering system is designed and installed for measuring electron scale turbulence (k ρs ∼ 40). A metal lens relay antenna is used for in-vessel beam focusing, and a beam diameter of less than 40 mm is achieved in the plasma core region. This antenna can be steered at an angle of 159 ○ ± 6 ○ , which almost covers the plasma radius. The estimated size of the scattering volume is ∼105 mm at the edge and 135 mm at the core, respectively. A 60 m corrugated waveguide is used to achieve a low transmission loss of ∼8 dB. A heterodyne detection system for millimeter-wave circuits with probing power modulation can distinguish the scattered signal from background noise.
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