Combining temporal scattering, depolarization, and RM variation measurements yields source-to-magneto-active-screen distances of ~AU to ~pc for six repeating FRBs, tentatively separating binary from SNR environments.
The linear fitting of RM vari- ation in two stages turns out to be 0.41 rad/m2/day and -1.18 rad/m2/day, respectively
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AU or pc? Inferring the distance of magnetized plasma near FRBs from propagation diagnostics
Combining temporal scattering, depolarization, and RM variation measurements yields source-to-magneto-active-screen distances of ~AU to ~pc for six repeating FRBs, tentatively separating binary from SNR environments.