  Magnetosheath jets are currently an important topic in the field of
magnetosheath physics. It is thought that 97~\% of the jets are produced by the
shock rippling at quasi-parallel shocks. Recently, large statistical studies of
magnetosheath jets have been performed, however it is not clear whether
rippling also produces jets found downstream of quasi-perpendicular shocks. We
analyze four types of events in the quasi-perpendicular magnetosheath with
signatures characteristic of magnetosheath jets, namely increased density
and/or dynamic pressure, that were not produced by the shock rippling: 1)
magnetic flux tubes connected to the quasi-parallel bow-shock, 2)
non-reconnecting current sheets, 3) reconnection exhausts and 4) mirror mode
waves. The flux tubes are downstream equivalents of the upstream traveling
foreshocks. Magnetosheath jets can impact the magnetopause, so knowing the
conditions under which they form may enable us to understand their signatures
in the magnetosphere.
