Methods of statistically estimating the characteristics of scatterers
from noisy data are proposed. The first approach is based on the Lippm
an-Schwinger (LS) equations. The estimator based on the method of maxi
mum posterior probability minimizes the appropriate non-quadratic func
tional. The latter includes the quadratic form of the discrepancy betw
een the estimated fields and experimental data, constraints imposed on
the inner fields, and apriori statistical information on the scattere
r. The second approach uses the Marchenko Newton-Rose (MNR) equation t
o estimate the inner field and the correlation function of reconstruct
ion errors. This equation implies the pulse regime. Now the estimate m
ay be obtained either directly from the LS equation or from the wave e
quation. The ''miracle'' phenomenon is analyzed: the scatterer estimat
e is independent of the inner field parameters-the position of the poi
nt source and the time of observation-which are chosen after solving t
he MNR equation. With this approach, the ''miracle'' takes place only
within the correlation domain of the errors in reconstructing the inne
r field.