A Space Time Functional Formalism for Turbulence

Cover A Space Time Functional Formalism for Turbulence
A Space Time Functional Formalism for Turbulence
Robert M Lewis
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, k_, . . . , t, k ) v o / | nJ J a, ... , cl v 1' 1* * n' n ; n=l n a .
v I | z J (t. , k. )dt n dk n . .. Dt dk X I v j* j y 1 1 n n ' j=l where c-n p (1+3) P (t n, k n, ... , t, k N 5 Z 1 (t 1, k 1 ), ... , 6z n (t n, k n : Now from (1+0) we see that lU (kk) kj J P^, ... , ^ = °> J=l, ... , n; and from this it follows that there exist functions Q „ such that 1' ' ' ' ' n _nr p a p -, C*5) P (t^k, ...^, k ) =TT 5 „ R " k k k K r (t, ,k. , ... , t, k ) From (Ul), we have P = 1 so that T may he
... represented in the form v*) r ^ = i + ]T sr/^ [\ P ; k v" 2k X v ]\, .. VPn ]T ^^A' • - d V k n • n=l The incompressihility condition (UO) now is automatically satisfied.
From (9) and (33) we see that the space-time correlation function (hi) U ■ (t 1, x 1, ... , V x n ) =(u ai (t 1, x 1 )... U\, Xn ) > 1* ' n is given by 1' ' n J 1* ' n For many purposes it is useful to transform (39) so that a characteristic Reynolds number appears rather than tne viscosity coefficient v. This can be done by introducing some appropriate characteristic correlation length r and characteristic velocity v .


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