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- W2080491368 abstract "The non-isothermal magnetohydorstatic equilibrium is studied in this paper, on the basis of two-dimensional solutions of an isothermal case[9]. We present two models of temperature distribution and derive the two relevant partial differential equations of non-isothermal magnetohydrostatic equilibrium. Using the solution of the isothermal case as an approximation of the 1st degree and choosing appropriate boundary conditions, we obtain several solutions of the equations with an iterative method numerically, and obtain the equilibrium configurations and the distributions of temperature and magnetic energy. From these results, we find that the equilibrium configurations will change obviously as the temperature changes from the isothermal case slightly. Change of the temperature may play an important role in producing relatively violent solar activities through instability." @default.
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- W2080491368 date "1992-10-01" @default.
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- W2080491368 title "Non-isothermal magnetohydrostatic equilibrium structure in the solar atmosphere" @default.
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- W2080491368 doi "https://doi.org/10.1016/0275-1062(92)90040-i" @default.
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