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Using data from the Voyager 1 and 2 CRS telescopes available on the webthrough the end of 2014 we have studied the intensity variations of terminationshock H nuclei and anomalous cosmic ray H and He nuclei as a function of radialdistance. In contrast to the inner part of the heliosheath where the intensityvs. radius profiles in the North and South heliosheaths are much different,these intensity vs. radius profiles, as well as the intensities themselves, aremore similar in the outer North and South heliosheaths as measured by V1 and V2respectively. In the N heliosheath, taken to be 27.6 AU thick beyond the HTScrossing distance of 94 AU, the intensities of termination shock particles andanomalous cosmic rays reach a maximum at between 110-112 AU or at a location~halfway between the termination shock and the heliopause. They then decreasemore or less continuously to an intensity ~2/3 of the maximum for eachcomponent just before the final dropout at ~121 AU, just inside the heliopause.This intensity-time behavior favors theories in which the acceleration and losseffects lead to a maximum near the middle of the heliosheath.

A Comparison of Radial Intensity Profiles of Termination Shock Particles  and Anomalous Cosmic Rays in the Outer North-South Heliosheaths Using CRS  data from V1 and V2