“…However, the advantages of the powerlaw scaling is it is applicable (where n = 0, 1/2 or 1) for the full range of St o and gives a slightly better correlation (e.g. see above, Laats (1966) and Laats and Frishman (1970), St o = 18, where R 2 xu ¼ 0:978 and 0.964 for power-law and exponential scaling, respectively). Moreover, the power-law seems to have a physical basis, especially in the regime St o J 200, which corresponds to the scaling of a variable density jet (see Chen and Rodi, 1980).…”