Scintillation timescale measurement of the highly active FRB20201124A

Abstract

Scintillation of compact radio sources results from the interference between images caused by multipath propagation, and probes the intervening scattering plasma and the velocities of the emitting source and scattering screen. In FRB20201124A, a repeating fast radio burst (FRB) which entered a period of extreme activity, we obtained many burst detections in observations at the upgraded Giant Metrewave Radio Telescope (uGMRT) and the Effelsberg 100\,m Radio Telescope. Bursts nearby in time show similar scintillation patterns, and we measure a scintillation timescale of $14.3\pm 1.2$\,min and $7\pm 2$\,min at Effelsberg (1370\,MHz) and uGMRT (650\,MHz), respectively, by correlating burst pair spectra. The scintillation bandwidth scaled to 1\,GHz is $0.5\pm 0.1$\,MHz, and the inferred scintillation velocity at Effelsberg is $V_{\mathrm{ISS}}\approx (59\pm 7)\sqrt{d_l/2\mathrm{kpc}}{\mathrm{km}\mathrm{s}}^{-1}$, higher than Earth's velocity for any screen beyond a lens distance of $d_l\gtrsim 400$pc. From the measured scintillation bandwidth, FRB20201124A has comparatively lower scattering than nearby pulsars, and is underscattered by a factor of $\sim 30$ or $\sim 1200$ compared to the NE2001 and YMW16 model predictions respectively. This underscattering, together with the measured scintillation velocity are consistent with a scattering screen more nearby the Earth at $d_l\sim 400$pc, rather than at the 2\,kpc spiral arm which NE2001 predicts to be the dominant source of scattering. With future measurements, the distance, geometry, and velocity of the scattering screen could be obtained through modelling of the annual variation in $V_{\mathrm{ISS}}$, or through inter-station time delays or interferometric observations. Scintillation/scattering measurements of FRBs could help improve Galactic electron density models, particularly in the Galactic halo or at high Galactic latitudes.

9 pages, 9 figures, Accepted for publication in MNRAS

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• FAST observations of an extremely active episode of FRB 20201124A: II. Energy Distribution
• Milliarcsecond localisation of the repeating FRB 20201124A
• The Large Dispersion and Scattering of FRB 20190520B are Dominated by the Host Galaxy
• First discoveries and localisations of Fast Radio Bursts with MeerTRAP: a real-time, commensal MeerKAT survey
• High frequency study of FRB 20180916B using the 100-m Effelsberg radio telescope
• Burst properties of the highly active FRB 20201124A using uGMRT
• A Comprehensive Analysis on Repeating Fast Radio Bursts
• Modelling Annual Scintillation Velocity Variations of FRB 20201124A
• Detection of a bright burst from the repeating FRB 20201124A at 2 GHz
• Solar System-scale interferometry on fast radio bursts could measure cosmic distances with sub-percent precision
• Atlas of dynamic spectra of fast radio burst FRB 20201124A