Nonthermal nuclear effects triggered in the solar carbon-nitrogen-oxygen (CNO) cycle by fast a particlesproducts of the pp chain reactions-are examined. The main attention is paid to 8.674-MeV a particles generated in the 7Li(p ,a )a reaction. Nonthermal characteristics o f these a particles and their influence on some nuclear processes are determined. It is found that the a-particle effective temperature is at a level of 1.1 MeV and exceeds the solar core temperature by 3 orders of magnitude. These fast particles are able to significantly enhance some endoergic (a ,p ) reactions neglected in standard solar model calculations. In particular, they can substantially affect the balance o f the p + n O a + l4N reactions due to an appreciable increase of the reverse reaction rate. It is shown that in the region R = 0.08-0.25 Ra the reverse a + 14N reaction can block the forward p + l70 reaction, thus preventing closing o f the CNO-II cycle, and increase the 170 abundance by a factor o f 2-155 depending on R. This indicates that the fast a particles produced in the pp cycle can distort running o f the CNO cycle, making it essentially different in the inner and outer core regions.