The axial merging method is one of the candidates to provide a center-solenoid-free start-up of high-beta spherical tokamak (ST) plasma. Two initially formed STs merge through magnetic reconnection in the presence of the guide (toroidal) magnetic field, which is perpendicular to the reconnection (poloidal) magnetic field. During ST merging start-up, electrons are effectively accelerated near the reconnection point where the reconnection electric field is almost parallel to the magnetic field. In order to evaluate the effectivity of this acceleration process on electron heating, the temporal and spatial distributions of generated energetic electrons are observed by a soft x-ray fast imaging system equipped on the UTST device. The energetic electrons were generated not only in the vicinity of the reconnection point but transiently in the inboard-side downstream region until the static electric field by charge separation grew to cancel the reconnection electric field component parallel to the magnetic field line. Adequate control of the downstream condition could enhance the generation of energetic electrons and provide a more effective conversion from the released magnetic energy to electron energy.

Experimental setup to achieve long-pulse magnetic reconnection in partially ionized plasmas was developed using the rotating magnetic field technique. Two field-reversed configuration plasmas were formed and sustained along the axial direction in the experimental vessel, and the quasi-steady magnetic reconnection condition with the ionization degree of the order of 1 % was maintained for more than 20 ms between the plasmas. Time duration of magnetic reconnection longer than the ion-neutral collision time and plasma parameters where the neutral particles possibly affect the reconnection process, were achieved. Reconnection events observed under the present experimental conditions were classified into three cases according to the ionization degree, and a new experimental regime for magnetic reconnection in partially ionized plasmas was successfully demonstrated.

A new closed-type experimental setup to achieve a long-pulse magnetic reconnection in weakly ionized plasmas was developed by using a rotating magnetic field (RMF) technique. The experimental setup has a cylindrical vacuum vessel in which two sets of four antennas are equipped to generate RMF which drives steady azimuthal electron current in two torus plasmas. This device provided a quasi-steady magnetic reconnection condition in weakly ionized plasmas with ionization fraction of less than 1%. The proposed experimental setup will extend the research area of laboratory reconnection experiments and be helpful to comprehend the reconnection process in weakly ionized plasmas such as solar chromosphere.