“…The various mechanisms of the pulses reported in passively MLFLs, such as CS, , large-energy solitons pulse, , dissipative solitons, − HML, , and soliton rain , indicate that passively MLFL is an ideal platform for studying the NLO of SA and soliton dynamics. , As an operation state between continuous wave (CW) and CS pulse, soliton rain is typically characterized by the fact that there will be a continuous spontaneous formation of new soliton pulses in the noise and drift at an almost constant rate until eventually converging to the cohesive soliton phase . Large-energy pulses typically have pulse widths on the order of nanoseconds, so their pulse energies are much higher than the energy limit of CS.…”