Probability density functions (PDFs) of the strain-rate tensor eigenva
lues are examined. It is found that the accepted normalization used to
bound the intermediate eigenvalue between +/-1 leads to a PDF that mu
st vanish at the end points for a non-singular distribution of strain
states. This purely kinematic constraint has led previous investigator
s to conclude incorrectly that locally axisymmetric deformations do no
t exist in turbulent flows. An alternative normalization is presented
that does not bias the probability distribution near the axisymmetric
limits. This alternative normalization is shown to lead to the expecte
d flat PDF in a Gaussian velocity field and to a PDF that indicates th
e presence of axisymmetric strain states in a turbulent field. Extensi
on of the new measure to compressible flow is discussed. Several earli
er results concerning the likelihood of various strain states and the
correlation of these with elevated kinetic energy dissipation rate are
reinterpreted in terms of the new normalization. Most importantly, it
is found that regions of axisymmetric expansion play a much more domi
nant role in the turbulent dissipation process than was previously bel
ieved.