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The angular broadening of compact radio sources observed through a mediumhaving turbulent density irregularities is usually estimated using the phasestructure function. We employ an exact formulation for the phase structurefunction that helps in obtaining an accurate estimate of angular broadeningwhen the baseline lengths are comparable to the inner scale of the turbulentspectrum.

Constraining the amplitude of turbulence in solar corona using observations of angular broadening of radio sources