  We calculate the production rates of Li6, Li7, Be9, B10 and B11 via
spallation of Carbon, Nitrogen and Oxygen nuclei by protons and alpha-particles
and by alpha-alpha fusion reactions. We include recent measurements of the
cross sections of alpha-alpha fusion reactions and find that the computations
yield rates of Li6 and Li7 production that are nearly a factor of two smaller
than previously calculated. We begin by using the `straight ahead'
approximation for the fragment energy and the `leaky-box' model for product
capture in the Galaxy. In addition we test the straight ahead approximation by
recalculating the production rates using an empirical description of the
fragment energy distribution and find that the results closely match. We have
also calculated the rates for various cosmic ray spectra and find that the
hardest spectra tested decrease the rates with CR CNO by approximately an order
of magnitude relative to our chosen standard. Finally we have computed the
Population I elemental ratios and the Population II scaling relations for our
standard and find that our computations predict an abundance of Lithium for a
given abundance of Beryllium that is 1/4 smaller than previously derived.
