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Information × Registration Number 0212U005695, 0112U005021 , R & D reports Title Interaction of plasma flow with obstacle: experimental study of multiscale dynamics in the solar wind streamlining around magnetosphere popup.stage_title Head Ivchenko Vasyl Mykolayovich, Registration Date 08-01-2013 Organization Taras Shevchenko Kiev university popup.description2 Investigation of statistical features of the magnetic field fluctuations in bound regions of Earth's magnetosphere, on different time scales, is carried out in this work. Measurements of Cluster-2 with interrogation frequency 22.5 Hz for 2004-2010 years and space vehicle "Interball-1" for 1996 - 1998 years have been used for the analysis. During these investigations we have studied the changes of shape and parameters of probability density function for magnetic field fluctuations for periods of presence of the satellite in magneto-layer, solar plasma wind and in region of magnetopause. We have considered the evolution of change of maximum of probability density function and investigated structure functions of different orders as characteristics of turbulent processes for different time scales. Investigation of structure functions of high orders helped us to determine the character of turbulent processes and study diffusion in the considered regions. We have found, that the highest intermittence is observed in the postshock region; for the middle magnetosheath the results of experimental data correspond to log-Poisson turbulent cascade model, and for the description of processes in SW plasma one can use the Iroshnikov-Kraichnan's model; in the boundary layers we have the superdiffusion processes. Product Description popup.authors Козак Людмила Володимирівна Могильчак Владислав Юрійович Парновський Олексій Сергійович Пилипенко Сергій Григорович Цупко Олександр Олександрович Черемних Олег Костянтинович popup.nrat_date 2020-04-02 Close
R & D report
Head: Ivchenko Vasyl Mykolayovich. Interaction of plasma flow with obstacle: experimental study of multiscale dynamics in the solar wind streamlining around magnetosphere. (popup.stage: ). Taras Shevchenko Kiev university. № 0212U005695
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Updated: 2026-03-21