Scattering variability detected from the circumsource medium of FRB 20190520B
S.K. Ocker, J.M. Cordes, S. Chatterjee, D. Li, C.H. Niu, J.W. McKee,, C.J. Law, R. Anna-Thomas

TL;DR
This study reports variable scattering times in a repeating FRB, revealing dynamic plasma conditions near the source that affect radio wave propagation and offer insights into the local environment of FRBs.
Contribution
It presents the first evidence of rapid scattering variability in a repeating FRB, linking it to inhomogeneous circumsource plasma and highlighting its impact on FRB observations.
Findings
Scattering times vary by up to a factor of two over minutes to days.
Scattering times can change significantly within a few minutes.
Variations are uncorrelated with dispersion and rotation measures.
Abstract
Fast radio bursts (FRBs) are millisecond-timescale radio transients, the origins of which are predominantly extragalactic and likely involve highly magnetized compact objects. FRBs undergo multipath propagation, or scattering, from electron density fluctuations on sub-parsec scales in ionized gas along the line-of-sight. Scattering observations have located plasma structures within FRB host galaxies, probed Galactic and extragalactic turbulence, and constrained FRB redshifts. Scattering also inhibits FRB detection and biases the observed FRB population. We report the detection of scattering times from the repeating FRB 20190520B that vary by up to a factor of two or more on minutes to days-long timescales. In one notable case, the scattering time varied from ms to less than 3.1 ms ( confidence) over 2.9 minutes at 1.45 GHz. The scattering times appear to be…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · GNSS positioning and interference · Radio Astronomy Observations and Technology
