“…ICE was early observed from fusion-born ion populations in pure deuterium and DT plasmas in JET [1][2][3][4] and TFTR [5,6], and from neutral beam injected (NBI) ions in TFTR [7]. Since 2017, ICE has been detected and analysed from NBI and fusion-born ions in the KSTAR [8][9][10], DIII-D [11][12][13][14][15][16], ASDEX-Upgrade [17][18][19][20][21], NSTX-U [22,23], JT-60U [24][25][26], TUMAN-3M [27][28][29], EAST [30][31][32][33] and HL-2A [34,35] tokamaks, and the LHD heliotron-stellarator [36][37][38][39][40][41]. The magnetoacoustic cyclotron instability (MCI) has been identified as the excitation mechanism for ICE through analytical studies [6,7,42] and simulations [8-10, 12, 38, 39, 43-46].…”