“…One dynamic phenomenon, the flapping motions of the tail current sheet, manifests in observations as dramatic variations of the main magnetic field component (tail-aligned, B x ) in the tail, often with the change in the B x sign, indicating a crossing of tail current central surface. Being known since first spacecraft measurements in the tail (Speiser and Ness, 1967), it is frequently observed in the active plasma sheet and is interesting both as a spectacular phenomenon (origin, properties, possibility to use as a diagnostic tool of active processes), as well as a tool to probe the sheet structure by crossing quickly across considerable portions of the current sheet (CS) thickness. There was a number of past studies which noticed their association with interplanetary shocks (McComas et al, 1986), with substorms and/or fast flows (Toichi and Miyazaki, 1976, Bauer et al, 1995, although counter-examples were also provided.…”