The monograph is devoted to the development of continuous models of turbulent environments - models that underlie the formulation and numerical calculations of tasks related to the formation, structure and evolution of various astro- and geophysical objects. Stochastic model approaches to relevant problems are considered as a reflection of self-organization processes in dissipative open systems. Examples of the occurrence of orders in various space objects and natural environments during their evolution are given. For researchers working in the fields of astrophysics, geophysics, planetary science, aeronomy and space research, as well as for senior students and graduate students of relevant specialties.