Toroidal ion temperature gradient (ITG) driven drift mode turbulence h
as been analyzed analyti- cally and numerically. By using weak nonline
arity arguments and random phase approximation, dynamic and wave kinet
ic equations are derived. Three different nonlinearities, namely ExB,
convective, and diamagnetic nonlinearities, play important roles in th
e turbulent spectral transfer. The power spectra of tile weak ITG-mode
turbulence are obtained analytically for \k\much greater than 1 and \
k\<1 ranges in the wave number space. Foward energy cascading due to c
onvective and diamagnetic nonlinearities will balance the inverse ener
gy cascading due to ExB nonlinearity at \k\approximate to 1/p(s) (k is
the wave number, p(s)=c(s)/omega(ci), where c(s) is the sound velocit
y and omega(ci) is the ion cyclotron frequency and results in energy c
ondensation at \k\approximate to 1/p(s). (C) 1996 American Institute o
f Physics.