Abstract. We review results from the most recent experiments in the past 2 decades in which magnetic reconnection has been generated and studied in controlled laboratory settings. As a whole, research on the fundamental physics of the reconnection process and its hydromagnetic consequences has been largely theoretical. Laboratory experiments are crucial for understanding the fundamental physics of magnetic reconnection since they can provide well-correlated plasma parameters at multiple plasma locations simultaneously, while satellites can only provide information from a single location at a given time in a space plasma. Thanks to the significant progress of data acquisition technology, the detailed magnetic field structures of the reconnection regions were measured and plasma acceleration and strong ion heating were identified. ]. In this recent work it is found that the observed reconnection rate can be explained by a generalized Sweet-Parker model, which incorporates compressibility, downstream pressure and the effective resistivity. The latter is often enhanced over its classical values in the collisionless limit. A significant implication of this result is that the generalized Sweet-Parker model is valid in certain 2-D reconnection cases with axisymmetric geometry. In MHD plasmas, the thickness of this thin current layer is found to be of the order of the ion gyroradius and the ion skin depth as well.