Abstract
On 29 March 1986 between 16:00 and 23:00 UT we observed the strong compact radio source 1827-360 as the plasma tail of comet Halley swept across the source. We noted the appearance of weak intensity fluctuations during the interval 17:00 to 19:00 UT when the Sun, the comet's nucleus and the radio source were accurately aligned. We interpret this behaviour as the result of diffraction of radio waves by electron-density irregularities in the plasma tail. At a distance 5.4 × 106 km downstream from the cometary nucleus the central part of the plasma tail contained electron density irregularities about 14 times as strong as those in the undisturbed solar wind.
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Slee, O., McConnell, D., Lim, J. et al. Scintillation of a radio source observed through the tail of comet Halley. Nature 325, 699–701 (1987). https://doi.org/10.1038/325699a0
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DOI: https://doi.org/10.1038/325699a0
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