A major difficulty facing the study of geomagnetic polarity reversals lies
in interpreting palaeomagnetic records of polarity transitions. These recor
ds are the sole source of information about what happens to the field as it
reverses. In addition to comparison of records of the same reversal from d
ifferent types of recorders to check for accuracy, we need some internal me
asure that can be used as a gauge of the temporal resolution provided by th
e data. This paper explores methods using the extent to which secular varia
tion is recorded in the full polarity intervals bounding polarity transitio
ns to estimate the temporal extent to which the transitional record should
be interpreted. Cumulative dispersion and two autocorrelation methods are e
valuated using datasets representative of different end-member palaeomagnet
ic records of secular variation and polarity transitions.