Collaboration between the mployees of the Institute of Mathematics and Mechanics of ANAS and employees of Shamakhi Astrophysical Observatory named after Nasreddin Tusi has started by building the models of the problems “Some solutions of Magnitohydrodynamic Transition Equations for Anisotropic Solar Wind Model”, “Distinctive Diversity of Sun’s Special Dances with Magnetic Field Effects” and “MHD Kelvin-Helmholtz Stabilization in anisotropic solar wind plasma”, to solve the nonlinear equations obtained. To this end, a working group was established with the participation of the employees of the Institute of Mathematics and Mechanics, doc. tech. sci. Elkhan Abbasov, doct. phys. math. sci., prof. Akbar Aliyev, doct. phys. math. sci., prof. Farman Mammadov and candidate phis. math. sci., ass. prof. Abdurrahim Guliyev. It was planned to consider the adequacy of the chosen model to the real conditions, the correct selection of the solutions of the obtained equations describing the process, and in some cases the possibility of solving the equations by numerical methods.

Workshops were held separately on the issues considered and wide discussions were held. During the discussion, it was discussed the principles of reflection of equations, initial and boundary conditions, simplification of the equations and selection of solutions, the statement of the problem, the well-posedness of the initial and boundary conditions of received differential equations were discussed and some advies on the rules of selection of solution were given.

All rights are reserved. Citing to www.imm.az is necessary upon using news.