In the previous work [32], we considered the phenomenon of "palindromes", which stands for a high probability of similar histograms to be found upon comparison of two data series: first, representing the results of measurements of [sup.239]Pu [alpha]-decay over
astronomical day (since 6 to 18 h by local, longitude, time) and, second, measured over astronomical night (since 18 to 6 h, in continuation of the first series) and inverted.