We present a general method for the reconstruction of the one-point Probabi
lity Distribution Function of the local aperture mass in weak lensing maps.
Exact results, that neglect the lens-lens coupling and departure from the
Born approximation, are derived for both the quasilinear regime at leading
order and the strongly nonlinear regime assuming the tree hierarchical mode
l is valid. We describe in details the projection effects on the properties
of the PDF and the associated generating functions. In particular, we show
how the generic features which are common to both the quasilinear and nonl
inear regimes lead to two exponential tails for P(M-ap). We briefly investi
gate the dependence of the PDE with cosmology and with the shape of the ang
ular filter. Our predictions are seen to agree reasonably well with the res
ults of numerical simulations and should be able to serve as foundations fo
r alternative methods to measure the cosmological parameters that take adva
ntage of the full shape of the PDF.