The suggestion that sunspot transition region oscillations are a typical fe
ature of the sunspot plumes is examined. The present observations show 3 mi
n oscillations in the umbra that end at the umbral rim. We find that sunspo
t plumes located above the umbra show these oscillations, in contrast to pl
umes above the penumbra. These two findings suggest that the oscillations m
ay be a property of the umbral transition region.