Acoustic time reversal is a robust means of retrofocusing acoustic energy,
in both time and space, to the original sound-source location. However, noi
se may limit the performance of a time-reversing array (TRA) at long source
-array ranges, or when the original-source or TRA-element power levels are
low. The operation of a TRA requires two steps (reception and transmission)
so both TRA-broadcast noise and ambient noise must be taken into account.
In this paper, predictions are made for how a simple omnidirectional noise
field influences the probability that the signal amplitude from a narrow-ba
nd TRA will exceed the noise at the TRA's retrofocus. A general formulation
for the probability of TRA retrofocusing, which can be used for TRA design
, is developed that includes: the variance of the noise field, the original
source strength, the TRA's element output power, the number of TRA element
s (N), and the propagation characteristics of the environment. This formula
tion predicts that a TRA's array gain tin dB) at the retrofocus may be as h
igh as + 10 log(10)(N) to + 20 log(10)(N) depending on the relative strengt
hs of the original source and the TRA's elements. Monte Carlo simulations i
n both a free-space environment and a shallow-ocean sound-channel environme
nt compare well to this probability formulation even when simple approximat
e parametric relationships for the appropriate Green's functions are used.
The dominant deviation between theory and simulation in the sound channel i
s caused by acoustic absorption. (C) 2001 Acoustical Society of America.