Abstract
Scintillation times and decorrelation bandwidths for the pulsars B0329+54, B1641–45, B1508+55 and B1919+21 are determined. The results are based on observations made with different instruments and at different radiofrequencies. All objects but the pulsar B1508+55 were detected to have more than one frequency scale. The obtained values of scattering parameters are not contrary in general to the Kkolmogorov form of density fluctuation spectrum.
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Kondratiev, V., Popov, M., Soglasnov, V. et al. Frequency Structure of Radio Scintillations for Several Pulsars. Astrophysics and Space Science 278, 43–46 (2001). https://doi.org/10.1023/A:1013177621936
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DOI: https://doi.org/10.1023/A:1013177621936