“…[1][2][3][4] However, many laboratory and space plasma boundaries are emissive, and the electrons emitted via process of thermionic emission, photoelectron emission and secondary electron emission (SEE) influence sheath structure dramatically, and consequently the near-wall heat flux and bulk plasma. [5][6][7][8] Therefore, understanding the characteristics of sheath near emissive surfaces is crucial for many plasma related applications and phenomena, e.g. emissive probe, 9,10 plasma thruster, 11,12 fusion reactor, 13,14 charging of spacecraft, 15,16 and dust levitation near lunar surface.…”