Extremely anisotropic scintillation
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A small number of quasars exhibit interstellar scintillation on time-scales less than an hour; their scintillation patterns are all known to be anisotropic. Here, we consider a totally anisotropic model in which the scintillation pattern is effectively one-dimensional. For the persistent rapid scintillator J1819+3845, we show that this model offers a good description of the two-station time-delay measurements and the annual cycle in the scintillation timescale. Generalizing the model to finite anisotropy yields a better match to the data but the improvement is not significant and the two additional parameters which are required to describe this model are not justified by the existing data. In contrast, our data for the persistent rapid scintillator PKS1257-326 are significantly better fit by a two-dimensional model with a major-to-minor axis ratio of 6 for the scintillation pattern. For J1819+3845, the totally anisotropic model predicts that the particular radio flux variations seen between mid-July and late August should repeat between late August and mid-November, and then again between mid-November and late December as the Earth twice changes its direction of motion across the scintillation pattern. If this effect can be observed then the minor-axis velocity component of the screen and the orientation of that axis can both be precisely determined. In reality, the axis ratio is finite, albeit large and spatial decorrelation of the flux pattern along the major axis may be observable via differences in the pairwise fluxes within this overlap region; in this case, we can also constrain both the major-axis velocity component of the screen and the magnitude of the anisotropy.
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Rapid interstellar scintillation of PKS 1257-326: Two-station pattern time delays and constraints on scattering and microarcsecond source structureBignall, Hayley; Macquart, Jean-Pierre; Jauncey, D.; Lovell, J.; Tzioumis, A.; Kedziora-Chudczer, L. (2006)We report measurements of time delays of up to 8 minutes in the centimeter-wavelength variability patterns of the intrahour scintillating quasar PKS 1257326, as observed between the VLA and the ATCA on three separate ...
Macquart, Jean-pierre; de Bruyn, A. (2009)We report the discovery of fast, frequency-dependent intensity variations from the scintillating intra-day variable quasar J1819+3845 at 21 cm which resemble diffractive interstellar scintillations observed in pulsars. ...
Geyer, M.; Karastergiou, A.; Kondratiev, V.; Zagkouris, K.; Kramer, M.; Stappers, B.; Grießmeier, J.; Hessels, J.; Michilli, D.; Pilia, M.; Sobey, Charlotte (2017)© 2017 The Authors Published by Oxford University Press. We measure the effects of interstellar scattering on average pulse profiles from 13 radio pulsars with simple pulse shapes. We use data from the LOFAR High Band ...