  Uncertainties in the Voyager data itself as well as the cross sections for
production of these secondaries at these low energies are an important
limitation on the estimates of the amount of matter traversed. We also attempt
a fit to the B observations at low energies by considering a source component
of B generated in 1.0 g/cm2 of matter near the sources but after acceleration.
This would be equivalent to a Nested LBM. In this model the V1 data below 40
MeV/nuc is now well fit. For Nitrogen, which is dominated by a source component
at these low energies, a fit to the data between 10-130 MeV/nuc can be obtained
with a N/O source ratio = 6.3 + 1.0% and a path length compatible with the H
and He propagation as noted above. This Voyager observation confirms earlier
measurements of a low N abundance in the cosmic ray source relative to what is
found for solar abundances, for example, where the N/O ratio is found to be
~12%.
