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Information × Registration Number 0215U001079, 0114U001945 , R & D reports Title Experimental consideration of turbulent properties of sunny and circumterrestrial plasma under cosmic "Strannik" project popup.stage_title Head Kostik R.I., Registration Date 16-01-2015 Organization Main Astronomical Observatory popup.description2 On the basis of analysis of surface observations of active solar photosphere and satellite data of ferroprobe magnetometers at crossing of solar plasma wind, magnetic area and magnetic pause it is set: 1. In the active regions of the Sun on different heights two modes of turbulence will be realized. Turbulent processes that is described by the model of Kolmogorov (izotropic turbulent processes) take place on small scales, and on large scales - by the model of Iroshnikov-Kraichnan (anisotropic turbulent processes). A transition takes place on the scales of mezogranulation. 2. Turbulent processes in plasma of solar wind are near to the model of Iroshnikov-Kraichnan, and in the middle of magnetic area described by izotropic loghpuasson's factorable model. 3. There are mainly reverse factorable processes in magnetic area. A magnetosphere behaves as a selforganized system with different characteristic scales. Product Description popup.authors Козак Л.В. Костик Р. І. Черемних О.К. popup.nrat_date 2020-04-02 Close