Statistically significant variations have been observed in the differential
flux of similar to 27-MeV anomalous cosmic ray (ACR) oxygen, helium, and p
rotons at the Voyager 1 spacecraft during 1998 and 1999 (at a helioradius o
f similar to 73 AU). The quasiperiodic variations are in phase, with oxygen
and helium having periods near 151 days, while protons exhibit a period of
similar to 146 days. The Voyager 1 ACRs vary by similar to 30% with respec
t to the trend, and similar galactic cosmic ray variations, if they exist,
must be less than similar to5%, probably much less. No similar, significant
periodicities have been detected for these same ACR species at Voyager 2 (
at 57 AU) during this period. We report on these and other periodicities in
the Voyager Low Energy Charged Particle experiment measurements and addres
s the possible connection between this similar to 151-day ACR periodicity a
nd the previously discovered similar to 154-day periodicities in solar flar
es, the interplanetary magnetic field, and other phenomena.