  Gallium solar neutrino experiments have historically used radiochemical
counting to determine the event rate. A detector which directly measures the
ejected electron and de-excitation gamma could reduce background counting rates
by way of a double-pulse technique. We find this reduction could be as large as
10 orders of magnitude in a 100 ton detector. In this process, the detector
measures the excited nuclear final state of the germanium after an electron
neutrino interacts with gallium nucleus through the charged-current
interaction. This results in a loss of approximately 90\% of the total neutrino
signal, but higher energy processes are less suppressed. The neutrinos
resulting from this higher energy selection are predominantly from the {}$^8$B
and {}$^7$Be solar neutrino fluxes.
