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.
E.3.Clumps in SNR The RM variations of FRBs could also be attributed to filaments in SNRs across the line of sight (J
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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.