Spatial Spikes of Intensity of the Atmospherically–distorted Images

At registration of astronomical objects through the turbulent atmosphere for large telescopes conditions will be usually realized, when the astronomical image represents from self a chaotic picture interleaved light and dark spots (speckle-strusture). In this connection, it is represented interesting to give an estimation of size of characteristic parameters of these areas. In given message the similar analysis will be carried out on the basis of treatment light spots of speckle-structure as the random spikes of intensity of the astronomical image.