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[en] Stationary solutions in the form of small-scale periodic cells in a plane perpendicular to the magnetic field are obtained in the framework of two-fluid magnetohydrodynamics. The solutions are established as a result of the development of thermal instability and represent a superposition of standing temperature waves. In solving the problem, an expression is used for a generalized heat source (including heating and radiative cooling) that forms a temperature transition region between the chromosphere and corona.
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