The main mechanism of radiocarbon 14 C creation in the Earth's atmosphere is ensured by cosmogenic irradiation with a yield of 472 g-mole/year (Roth & Joos, 2013) in the reaction 14 N(n,p) 14 C. The generated isotope of 14 C is assimilated in the biomass and decays within it (T 1/2 = 5700 years) that allows us to date the age of investigated organic materials. Discovery of short-term secular fluctuations of radiocarbon in tree rings (Suess, 1965) and its correlation with sun spot number had raised questions that should be eliminated to explain the nature of the phenomenon. In addition to the solar mechanism of fluctuations, the hypothesis of short-term 14 C variation under thunderstorm generated neutrons in fusion reaction 2 H + 2 H → 3 He + n (due to acceleration of deuterium ions at lightning discharges) with a yield of ≃2.5 MeV neutrons (Libby & Lukens, 1973) was proposed. But the deuterium concentration in the atmospheric H 2 O vapor is small (1 2 H nucleus per ∼10 4 1 H nuclei) (Rozansky & Sonntag, 1982;Gerst & Quay, 2000), and the maximal electric field strength inside the thunderclouds (∼1 × 10 6 V/m) (Winn et al., 1974;Gunn, 1948) is too small for evident neutron generation, which results in negligible neutron creation (Babich, 2006); in conclusion, the fusion cannot be responsible for short-term radiocarbon fluctuation. Nevertheless, indications of the low-rate fusion are obtained; so, the authors of the experiment at the High Altitude Research Laboratory (India) registered that 2.45 MeV neutrons correlated with lightning strokes (Ishtiaq et al., 2016).The first evidence of thunderstorm neutron enrichment was obtained in high-altitude Himalayas experiment (Shah et al., 1985). The enrichment of neutron fluxes, γ-and X-rays in correlation with thunderstorms were also registered in the following experiments (as: