Short term distribution of signal fluctuations due to troposheric scin
tillation (in decibels) is usually modelled as Gaussian. For long term
distribution, this results in a symmetrical distribution function. Ho
wever, various experiments have shown a significant asymmetry in long
term distribution for strong scintillations. It is shown that the obse
rved asymmetry follows directly from theory, if a different modelling
approach is applied.