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We have derived background corrected intensities of 3-50 MeV galacticelectrons observed by Voyager 1 as it passes through the heliosheath from 95 to122 AU. The overall intensity change of the background corrected data from theinner to the outer boundary of the heliosheath is a maximum of a factor ~100 at15 MeV. At lower energies this fractional change becomes less and the correctedelectron spectra in the heliosheath becomes progressively steeper, reachingvalues ~ -2.5 for the spectral index just outside of the termination shock. Athigher energies the spectra of electrons has an exponent changing from thenegative LIS spectral index of -1.3 to values approaching zero in theheliosheath as a result of the solar modulation of the galactic electroncomponent. The large modulation effects observed below ~100 MV are possibleevidence for enhanced diffusion as part of the modulation process for electronsin the heliosheath.

A Galactic Cosmic Ray Electron Intensity Increase of a factor of up to  100 At Energies between 3 and 50 MeV in the Heliosheath between the  Termination Shock and the Heliopause Due to Solar Modulation As Measured by  Voyager 1