https://nova.newcastle.edu.au/vital/access/ /manager/Index en-au 5 https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:36 . Since the Taylor microscale Reynolds number R-lambda is approximately constant (similar or equal to450) along the jet axis, the structure functions and spectra also collapse approximately when the normalization uses either the Kolmogorov or integral length scales. Over the dissipative range, the best collapse occurs when Kolmogorov variables are used. The use of and the integral length scale L provides the best collapse at large separations. A measure of the quality of collapse is given. (C) 2005 American Institute of Physics.]]> Wed 11 Apr 2018 15:49:01 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:3133 Wed 11 Apr 2018 09:22:36 AEST ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:20713 Sat 24 Mar 2018 08:06:21 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:5159 Sat 24 Mar 2018 07:49:41 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:343 Sat 24 Mar 2018 07:42:28 AEDT ]]> https://nova.newcastle.edu.au/vital/access/ /manager/Repository/uon:4754 Sat 24 Mar 2018 07:21:07 AEDT ]]>