  Collisionless space plasma turbulence can generate reconnecting thin current
sheets as suggested by recent results of numerical magnetohydrodynamic
simulations. The MMS mission provides the first serious opportunity to check if
small ion-electron-scale reconnection, generated by turbulence, resembles the
reconnection events frequently observed in the magnetotail or at the
magnetopause. Here we investigate field and particle observations obtained by
the MMS fleet in the turbulent terrestrial magnetosheath behind quasi-parallel
bow shock geometry. We observe multiple small-scale current sheets during the
event and present a detailed look of one of the detected structures. The
emergence of thin current sheets can lead to electron scale structures where
ions are demagnetized. Within the selected structure we see signatures of ion
demagnetization, electron jets, electron heating and agyrotropy suggesting that
MMS spacecraft observe reconnection at these scales.
