Abstract
Interstellar turbulent plasma can be considered to be a radio astronomy antenna—an interstellar diffraction grating, with an aperture size roughly equal to the scattering-disk radius, R sc = z eff θ sc ≈ 1 AU (where z eff is the effective distance and θ sc the scattering angle). The angular resolution of this interstellar diffraction grating is of the order of ϕ dif = 1/(k R sc ). A single ground-based radio telescope can be used as a receiver for the interstellar diffraction grating. The grating’s parameters can be obtained only from observations on a system of interferometers with an angular resolution comparable to the scattering angle θ sc . The range of baselines necessary to determine the parameters of the grating is close that of the Earth-space RadioAstron interferometer.
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Original Russian Text © V.I. Shishov, 2010, published in Astronomicheskiĭ Zhurnal, 2010, Vol. 87, No. 8, pp. 789–794.
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Shishov, V.I. Interstellar scintillations and nanoarcsecond resolution in radio astronomy. Astron. Rep. 54, 724–729 (2010). https://doi.org/10.1134/S1063772910080056
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DOI: https://doi.org/10.1134/S1063772910080056