Fast radio burst dispersion measures exhibit scaling consistent with two-dimensional Kolmogorov turbulence in the intergalactic medium, constraining the outer scale to several megaparsecs.
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Polarization position angles of repeating FRBs are Gaussian distributed with no periodicity, arising from geometric projection in a stochastically varying magnetosphere that also explains non-repeating FRBs.
Author contributes to SPOTLIGHT collaboration using modern radio tech to search for fast radio transients and pulsars.
citing papers explorer
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Utilizing Dispersion Measure of Fast Radio Bursts to Probe the Intergalactic Medium Turbulence
Fast radio burst dispersion measures exhibit scaling consistent with two-dimensional Kolmogorov turbulence in the intergalactic medium, constraining the outer scale to several megaparsecs.
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Random Polarization Position Angle Behaviors across Bursts of Repeating Fast Radio Bursts
Polarization position angles of repeating FRBs are Gaussian distributed with no periodicity, arising from geometric projection in a stochastically varying magnetosphere that also explains non-repeating FRBs.
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Searching For Fast Radio Transients And Radio Pulsars Using SPOTLIGHT
Author contributes to SPOTLIGHT collaboration using modern radio tech to search for fast radio transients and pulsars.