  Using Leaky Box Model propagation calculations for H nuclei and a Monte Carlo
diffusion propagation model for electrons, starting from specific source
spectra, we have matched the observed LIS spectra of these cosmic rays measured
by Voyager at lower energies and AMS-2 at higher energies, a range from ~10 MeV
to ~1 TeV. The source spectra required are very similar rigidity spectra. Below
~6-10 GV the source spectra for both particles are ~P-2.25 and above 10 GV the
spectra are ~P-2.36-2.40. This break in the source spectral index is not seen
for He and C nuclei in a match of Voyager and AMS-2 intensities both of which
have source rigidity spectra with an index ~-2.24 throughout the entire range
of measured energies from ~10 MeV//nuc to ~1 TeV/nuc. The absolute source
intensities of electrons and H nuclei are derived and the source ratio of
accelerated electrons to H nuclei is between 2-5%. The total number of
accelerated electrons is much greater than that for protons, however, because
the accelerated electron spectrum extends down to ~1-2 MV rigidity whereas the
H nuclei spectrum cannot be observed below ~50-100 MV because of ionization
energy loss. Most of these low energy electrons escape from the galaxy forming
an intergalactic background.
