Characterisation of the reconnection exhaust event. From top to bottom: the magnetic field magnitude, B (panel a); the magnetic field components in the LMN coordinates system (panel b); the solar wind speed, V_sw (panel c); the solar wind velocity components in the LMN coordinates system (panel d); the proton number density, n_p (panel e); and the proton temperature, T_p (panel d). In panels c and d, the black lines represent the reconnection model predictions according to Eq. (3). The left (right) dashed line indicates the reference point used for the prediction in the leading (trailing) portion of the exhaust.