Measurements from the polar-orbiting S3-3 satellite show that energetic ions frequently precipitate with isotropic pitch angle distributions at auroral latitudes on the dayside. We propose that this precipitation results from non-guiding center motion of radiation belt ions that drift into the magnetopause current sheet. We also propose that the ion precipitation and flows of energetic ions observed in the magnetosheath originate together within the magnetopause current sheet. Ions ejected from the magnetopause toward the earth flow along open field lines that are adjacent to the separatrix between open and closed field lines. Those ejected into the magnetosheath flow along field lines that are connected to the geomagnetic field and adjacent to the separatrix between the connected field lines and purely magnetosheath fields lines. These proposals are tested by comparing the S3-3 observations of precipitating ions with previously analyzed ISEE 1 observations of energetic ions obtained near the magnetopause and in the magnetosheath. The S3-3 observations imply that the region of ion precipitation is often continuous as a function of local time. This suggests that at least on the dayside there is often a continuous shell of magnetospheric ions within the magnetosheath flowing from the magnetosphere. These ions are likely an important source for energetic ions in the interplanetary medium. ¿American Geophysical Union 1987