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- W1657923067 abstract "A computer code “SOLAR WIND DYNAMICS” for MHD simulation of non-stationary developing 3D processes in the solar wind is suggested. The solution is constructed in Lagrange's approach. The code calculates and shows in a clear form (as a movie) the well-known dynamical processes in the solar wind: high-speed streams of different origin, quasi-shock fronts, rarefaction regions, magnetic field spirals. Some empirical regressions are introduced. This code could be used for the real time forecast of the solar wind disturbances and the level of the geomagnetic activity on the base of the solar magnetic field measurements. The code could be a useful tool for persons, who are interested in the solar-terrestrial predictions and the interplanetary dynamics modeling of the inner and middle heliosphere. THE CODE IS AVAILABLE UPON REQUEST." @default.
- W1657923067 created "2016-06-24" @default.
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- W1657923067 date "1992-01-01" @default.
- W1657923067 modified "2023-09-27" @default.
- W1657923067 title "THE MODELING OF DYNAMICAL PROCESSES IN THE SOLAR WIND BY THE METHOD OF MACROPARTICLES" @default.
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- W1657923067 doi "https://doi.org/10.1016/b978-0-08-042049-3.50125-3" @default.
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