Loitsyansky's integral, I, is important because it controls the rate of dec
ay of kinetic energy in freely-evolving, isotropic turbulence. Traditionall
y it was assumed that I is conserved in decaying turbulence and this leads
to Kolmogorov's decay law, u(2) similar to t(-10/7). However, the modern co
nsensus is that I is not conserved, which is a little surprising since Kolm
ogorov's law is reasonably in line with the experimental data. This discrep
ancy led Davidson (2000 J. Fluid Mech. submitted) to reassess the entire pr
oblem. He concluded that, for certain initial conditions, which are probabl
y typical of wind tunnel turbulence, freely evolving turbulence reaches an
asymptotic state in which the variation of I is negligible, a conclusion wh
ich is at odds with the predictions of certain closure models. In this revi
ew we revisit this debate. We explain why the widespread belief in the time
dependence of I owes much to a misinterpretation of Batchelor and Proudman
's original analysis (1956 Phil. Trans. R. Soc. A 248 369). Indeed, a surve
y of the experimental and numerical data shows that there is little evidenc
e for significant long-range pressure forces of the type which underpin the
supposed variation of I. Interestingly, Batchelor and Proudman reached the
same conclusion almost half a century ago. We conclude by extending the id
eas of Loitsyansky and Kolmogorov to MHD turbulence. We note that there exi
sts a Loitsyansky integral for MHD turbulence (Davidson 1997 J. Fluid Mech.
336 123) and show that this leads to energy decay laws which coincide with
the experimental data.