The classical theory of detection using the Neyman-Pearson principle i
s applied to stratosphere-troposphere (ST) radar signals. It is extend
ed to provide information regarding the detection of weak signals whic
h complements the detectability method usually employed in ST radar st
udies. It is shown that for ST radar signals of low amplitude and a de
tectability around 3 (a value commonly invoked in literature), the pro
bability of detection is about equal to the probability of false alarm
. The question of threshold detectability is also discussed. Spectral
moments errors are evaluated by a method which is an extension of the
analytical method of estimation developed by Miller and Rochwarger and
the results compared to other statistical and analytical models. As a
lready known, three factors can affect the error on the estimated para
meters: the signal-to-noise ratio, the spectral width and the incohere
nt integration number. For high signal-to-noise ratios, analytical res
ults are in good agreement with Barrick's and Denenberg's theoretical
models and with Yamamoto's statistical one. For low signal-to-noise ra
tios, the spectral parameters are more sensitive to the selected model
but overall variability is similar.