Characteristic properties of outflows from the neutron-star remnant for the fiducial ξ_TS = 1 case. The meridional plane is shown at time ﹩\bar{t}=184\,{\rm{ms}}﹩. Left to right: inverse plasma beta, β⁻¹, magnetic-field strength, ∣B∣, poloidal-field strength, ﹩| {B}^{{\rm{pol}}}| =\sqrt{{B}^{2}-{B}_{\phi }{B}^{\phi }}﹩, entropy per baryon, s, and the asymptotic Lorentz factor, W_∞, of unbound material at infinity. Streamlines in the ∣B∣ and W_∞ panels indicate the poloidal magnetic-field and velocity-field structures, respectively. Cyan contours represent densities ρ of 10¹⁴, 10¹³, 10¹², 10¹¹, and 10¹⁰ g cm⁻³.