Abstract. We report an ion-scale magnetic flux rope (the size of the flux rope is ∼ 8.5 ion inertial
lengths) at the trailing edge of Kelvin–Helmholtz (KH) waves observed by the Magnetospheric
Multiscale (MMS) mission on 27 September 2016, which is likely generated by
multiple X-line reconnection. The currents of this flux rope are highly
filamentary: in the central flux rope, the current flows are mainly parallel
to the magnetic field, supporting a local magnetic field increase at about
7 nT, while at the edges the current filaments are predominantly along the
antiparallel direction, which induce an opposing field that causes a
significant magnetic depression along the axis direction
(> 20 nT), meaning the overall magnetic field of this flux
rope is depressed compared to the ambient magnetic field. Thus, this flux
rope, accompanied by the plasma thermal pressure enhancement in the center,
is referred to as a crater type. Intense lower hybrid drift waves (LHDWs) are
found at the magnetospheric edge of the flux rope, and the wave potential is
estimated to be ∼ 17 % of the electron temperature. Though LHDWs
may be stabilized by the mechanism of electron resonance broadening, these
waves could still effectively enable diffusive electron transports in the
cross-field direction, corresponding to a local density dip. This indicates
LHDWs could play important roles in the evolution of crater flux ropes. Keywords. Magnetospheric physics (magnetopause, cusp, and boundary layers; solar wind–magnetosphere interactions)