ПОИСК СЛЕДОВ ТЯЖЕЛЫХ И СВЕРХТЯЖЕЛЫХ ЭЛЕМЕНТОВ В МЕТЕОРИТАХ

摘要

In this case their relative intensity (at an energy of 2.5 GeV/nucleon) is nearly 10-20 times less than that in previous enperiments. The analysis made in this paper shows that the search and identification of the tracks of superheavy cosmic nucle:should be carried out using crystals located up to 1-2 cm from the preatmospheric surfacre of meteorities.