The stationary analytic MHD model of the stationary axissymmetric current sheet in the solar wind is built. The current sheet is bounded by magnetic separatrixes that separate open and closed magnetic field lines. Powerful separatrix currents flow along the boundaries of the current sheet. The separatrix currents are stronger than current in the vicinity of the neutral line of the global current sheet. The model can be used to describe a heliospheric plasma sheet or a part of current system located near it.
52.30.Cv Magnetohydrodynamics
95.30.Qd Magnetohydrodynamics and plasmas
94.30.Kq Electric fields, field-aligned currents and current systems, and ring currents
$^1$Space Research Institute RAS\
$^2$Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN)
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