Spectral exponent
The symmetries of the governing equations developed in the previous courses (see source of complexity courses) can be used in order to perform the theoretical expression of spectral exponent β.
In the case of turbulence, considering the energy flux :

Where
and
If it is scale invariant
, hence
Kolmogorov 1941[1] derived the first scaling law :

A similar scaling analysis in Fourier space yields to the famous
derived by Obukhov 1941 :
