  The original 110 year long 27-day Recurrence Index (original R27) was
published more than forty years ago. That index, based on the autocorrelation
of consecutive 27-day sets of the geomagnetic aa-index, is a measure of the
cycle-to-cycle stability of high speed solar wind structure. During an effort
to extend the index, it was discovered that the index could be significantly
strengthened by pre-smoothing the geomagnetic aa-index listing used as input. A
revised index (revised R27) is presented which clearly shows periods of long
term stable solar wind structure toward the end of every sunspot cycle over the
last 150 years. The extension of R27 over an interval including the greater
part of the space age enables the updating of various studies of long-term
solar wind variability based on R27, as well as comparison of R27 with more
recently-developed solar-terrestrial parameters.
