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Magnetohydrodynamics describes dynamics in electrically conductive
fluids. These occur in our environment as well as in our atmosphere
and magnetosphere, and play a role in the sun's interaction with
our planet. In most cases these phenomena involve turbulences, and
thus are very challenging to understand and calculate. A sound
knowledge is needed to tackle these problems. This work gives the
basic information on turbulence in nature, comtaining the needed
equations, notions and numerical simulations. The current state of
our knowledge and future implications of MHD turbulence are
outlined systematically. It is indispensable for all scientists
engaged in research of our atmosphere and in space science.
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