Dispersion and rotation measures from fast radio burst (FRB) host galaxies based on the TNG50 simulation

Open Access

Fig. 6

Median of the different magnetic field components’ ratios to the total magnetic field ( $B_{component}^{2} / B_{total}^{2}$ $B_{{\rm{component}}}^2/B_{{\rm{total}}}^2$ , where the components are azimuthal, radial, and vertical) as a function of redshift (top). Distribution width of the average of the signed magnetic field strength maps as a function of redshift (bottom).

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