The book deals with the development of continual models of
turbulent natural media. Such models serve as a ground for the
statement and numerical evaluation of the key problems of the
structure and evolution of the numerous astrophysical and
geophysical objects. The processes of ordering (self-organization)
in an originally chaotic turbulent medium are addressed and treated
in detail with the use of irreversible thermodynamics and
stochastic dynamics approaches which underlie the respective
models. Different examples of ordering set up in the natural
environment and outer space are brought and thoroughly discussed,
the main focus being given to the protoplanetary discs formation
and evolution.
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