On vortex flow structures in the outer heliosphere.

Physics

Scientific paper

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Scientific paper

The vortex flow pattern in the outer heliosphere is calculated on the basis of hydrodynamical equations. Quantitative solution in cylindrical coordinates is used. Moving vortices may be formed due to the heliolatitudinal solar wind velocity dependence and nonstationary boundary conditions near the Sun. The flow pattern consists of a system of "cyclones" and "anticyclones".

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