  The contribution to the local cosmic-ray flux from the Geminga supernova is
calculated assuming shock acceleration to 10^14 eV in a remnant which was
formed several 10^5 years ago along with the Geminga pulsar. The particles are
propagated to Earth using a simple diffusion model. In the region below the
knee in the spectrum, it is found the supernova may contribute 10% of the local
cosmic-ray flux, assuming plausible explosion parameters. The contribution to
the amplitude of the anisotropy is not in conflict with the data in this energy
region.
