2022
DOI: 10.1088/1361-6587/ac7892
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First observation and interpretation of spontaneous collective radiation from fusion-born ions in a stellarator plasma

Abstract: During bursty MHD events, transient ion cyclotron emission (ICE) is observed from deuterium plasmas in the Large Helical Device (LHD) heliotron-stellarator. Unusually, the frequencies of the successive ICE spectral peaks are not close to integer multiples of the local cyclotron frequency of an energetic ion population in the likely emitting region. We show that this ICE is probably driven by a subset of the fusion-born protons near their birth energy EH = 3.02MeV. This subset has a kinetic energy component par… Show more

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Cited by 9 publications
(8 citation statements)
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“…An approximately linear relationship between the concentration of fusion-born alpha particles, √ n α /n e , (where n α is the alpha particle density, n e is the electron density), and ICE growth rate was predicted by MCI by theories and simulations [54,56], which explained the results of JET D-T experimental result. Furthermore, experimental results in TFTR [49], AUG [22,23,25], START [27], LHD [37,39], and KSTAR [18] have been attributed to the MCI [54,56]. Recently, a new collective cyclotron resonant process between fast ions and thermalizing fusion-born alpha particles through MCI is predicted by simulation [55], which would affect the transport of helium ash in fusion plasmas.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…An approximately linear relationship between the concentration of fusion-born alpha particles, √ n α /n e , (where n α is the alpha particle density, n e is the electron density), and ICE growth rate was predicted by MCI by theories and simulations [54,56], which explained the results of JET D-T experimental result. Furthermore, experimental results in TFTR [49], AUG [22,23,25], START [27], LHD [37,39], and KSTAR [18] have been attributed to the MCI [54,56]. Recently, a new collective cyclotron resonant process between fast ions and thermalizing fusion-born alpha particles through MCI is predicted by simulation [55], which would affect the transport of helium ash in fusion plasmas.…”
Section: Introductionmentioning
confidence: 99%
“…Through comparing the detected frequency and f ci , the ICE was located around the outer edge midplane of the plasma and was believed to be excited by deeply trapped alpha particles reaching the plasma edge. Subsequently, a significant amount of research has been conducted on ICE in tokamaks, including JT-60U [12][13][14][15], KSTAR [16][17][18], TUMAN-3M [19,20], ASDEX-U [21][22][23][24][25], EAST [26], START [27], MAST [28], JET [29] NSTX/NSTX-U [30,31] and DIII-D [32][33][34][35], stellarators, including W7-AS [36] and LHD [37][38][39][40], and field reversed configuration C-2U device [41,42]. ICE is located around both the edge and the core of the plasma, and is destabilized by EP from D-T and D-D fusion reaction, neutral beam injection (NBI), and plasma heating in the ion cyclotron range of frequencies.…”
Section: Introductionmentioning
confidence: 99%
“…Typical edge ICE observed in confined magnetic fusion devices, such as JET [4][5][6], JT60U2 [7,8], TFTR [9,10], ASDEX Upgrade [11], KSTAR [12,13], DIII-D [14,15], LHD [16], NSTX and EAST [17]. ICE from the plasma core has been reported in ASDEX Upgrade [18], DIII-D [14,19], JFT-2 M [20], JT60U2 [8], TUMAN-3 M [21], NSTX-U [22] and EAST [23] Tokamak.…”
Section: Introductionmentioning
confidence: 99%
“…ICE is widely observed from MCF plasmas. In addition to historical observations from the TFR [5] and JET [6,7] tokamaks, and from deuterium-tritium plasmas in JET [8,9] and TFTR [10], ICE has recently been reported and analyzed from the KSTAR [2,[11][12][13], JT-60U [14,15], DIII-D [16,17], ASDEX-Upgrade [18][19][20][21], TUMAN-3M [22,23], NSTX-U [24,25] and EAST [26] and JET [27] tokamaks, and from LHD [3,4,[28][29][30]. ICE is under consideration as a fast-ion diagnostic for ITER [31][32][33]; it is also observed from solar-terrestrial plasmas [34][35][36][37][38], and may be present downstream of supernova remnant shocks [39].…”
mentioning
confidence: 99%
“…The thermal majority and energetic NBI ions are often of the same species. For example, the NBI ions are sub-Alfvénic deuterons at 80 to 100 keV in KSTAR deuterium plasmas [2], super-Alfvénic and sub-Alfvénic protons at 40 keV in LHD hydrogen plasmas [3], and sub-Alfvénic deuterons at 70 keV in LHD deuterium plasmas [4,30].…”
mentioning
confidence: 99%