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- W2010672264 abstract "Abstract A class of exact solutions to the steady, two-dimensional magnetohydrodynamic equations ina cylindrical geometry is presented. These may model both closed and open magnetic structures found in the solar atmosphere. For closed structures, it is found that increasing the flow speed causes the summit of the arcade of closed magnetic fieldlines to rise. Parameter ranges also exist where the solution has regions of open and closed field, and so the solutions may be relevant for modelling flows in solar magnetic structures such as coronal streamers, X-ray bright points coronal plumes and coronal holes." @default.
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- W2010672264 modified "2023-10-14" @default.
- W2010672264 title "Steady flows in solar magnetic solutions structures-a class of exact MHD solutions" @default.
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- W2010672264 doi "https://doi.org/10.1080/03091929108227782" @default.
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