Low-frequency turbulence has been studied in a plasma embedded in a pu
re toroidal magnetic field. A study of the variation of the spectral c
haracteristics of the low-frequency turbulence with the variation in n
u(in)/OMEGA(i) has been carried out with two different sets of density
and potential profiles. The spectral relation between density and pot
ential fluctuations indicates that the Rayleigh-Taylor instability exc
ites fluctuations in the long wavelength region, while the Rayleigh-Ta
ylor driven drift instability is responsible for the short wavelength
regime for nu(in)/OMEGA(i) much less than 1. Spectral characteristics
observed in regions where density gradients are parallel to gravity ar
e similar to the case where density gradients are antiparallel to the
gravity and support the view that the fluctuations generated in the ba
d curvature region are transported to the good curvature region. The r
esults are in agreement with theoretical predictions, numerical simula
tions, in situ measurements, and other laboratory experiments on drift
and Rayleigh-Taylor instabilities. For nu(in)/OMEGA(i) greater-than-o
r-equal-to 1, the spectral characteristics change and may correspond t
o the collisional gradient drift instability or the cross-field instab
ility.