Notes. The first five columns after the periods delimiting the streams are the averages over the stream duration of the solar wind speed (V_SW), proton number density (n), proton temperature (T_p), magnetic field magnitude (B), and Alfvén speed (V_A). θ_BV is the angle between the mean magnetic field and the mean solar wind speed. z_±^rms are the root mean square amplitudes of the Elsasser variables. ⟨C_vB⟩ is the correlation between velocity and magnetic fluctuations. Finally, σ_r = −2z₋ ⋅ z₊/(z₊² + z₋²) is the normalized residual energy. For these last four quantities, fluctuations and Elsasser fields were computed by removing a 1 h running average.