Phase spiral at different Galactocentric radii with Gaia DR3 data. The panels show the vertical projection of phase space (Z–V_Z) coloured by median V_ϕ. We only use stars with |ϕ|< 20deg. The regions have a total radial width of 1 kpc and their centres are separated by the same amount. We used bins of ΔZ = 0.02 kpc and ΔV_Z = 1 km s⁻¹. The colour-map ranges correspond to the percentiles 30 and 70 of the distribution of V_ϕ in each volume in order to maximise the appearance of the spiral. We indicate the number of stars in the bottom part of the panels.