The characteristics of noise in fiber-optic gyros are analyzed quantit
atively. Based on its physical characteristics and on autocorrelation
function evidence, the noise is modeled as the addition of fractal Bro
wnian motion (FBM) and Gaussian white noise (GWN). The value of self-s
imilarlity parameter H in FBM and the intensity of GWN, sigma(w), in t
he model are robustly determined with an algorithm based on an orthono
rmal wavelet transform, which demonstrates well the coexistence of the
long-and short-term correlation components of the gyro noise. Moreove
r, it is revealed that FBM dominates the gyro noise, whereas the GWN i
s minor. (C) 1997 Optical Society of America.