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Understanding the outer heliospheric interface is a major challenge,especially in the light of recent observations by the IBEX and Voyagermissions. We present further details on a new required theoretical correctionthat has been identified as substantial in a recent paper, the so-called sourcedepletion effect. These results complement and expand earlier calculations oftransit-time delays by presenting global skymaps of Energetic Neutral Atoms(ENAs) calculated with the depletion correction, comparing them with skymapscalculated without these corrections. Our results demonstrate that thedepletion correction is critical for interpreting IBEX-Hi ENA fluxes generatedin the inner heliosheath, and that any attempt to reconstruct the shape of theheliospheric boundary needs to include the depletion correction, unlessarriving at considerably erroneous results.

Modeled IBEX/INCA skymaps including the keV-ENA source extinction in the outer heliosphere