Toroidal ion temperature gradient (ITG) driven drift mode turbulence h
as been analyzed analytically and numerically. By using weak nonlinear
ity arguments and random phase approximation, dynamic and wave kinetic
equations are derived. It is found that three different nonlinearitie
s, namely E x B, convective and diamagnetic nonlinearities, play impor
tant role in the turbulent spectral transfer. The power spectra of the
weak ITG-mode turbulence are obtained analytically for \k\ much great
er than 1 and \k\ < 1 ranges in the wave number space. It is shown tha
t forward energy cascading due to convective and diamagnetic nonlinear
ities will balance the inverse energy cascading due to E x B nonlinear
ity at \k\ approximate to 1/rho(s) (k is wave number, rho(s), (c(s)/om
ega(ci)) c(s) is the sound velocity and omega(ci) is the ion cyclotron
frequency) and results in energy condensation at \k\ approximate to 1
/rho(s).