A method of compensating the pulse profiles of pulsars for distortion by interstellar scattering, and restoration of their original shape, width and time position, is proposed. Its validity is investigated for the simplest form of scattering, corresponding to a thin screen. As a practical realization, low-frequency profiles of the pulses of PSR 0531 + 21 and 0136 + 57 are obtained.
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Kuz’min et al. (1993) studied this question.
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