Abstract
By employing a nonholonomic description of the governing equations, the complex lamellar motion of a viscous, incompressible and perfectly conducting dusty fluid is discussed, and some results of physical importance are derived.
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Singh, S.N., Tiwari, H.S. & Singh, H.P. Some geometric properties of a dusty fluid in MFD flows. Astrophys Space Sci 105, 237–244 (1984). https://doi.org/10.1007/BF00651077
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DOI: https://doi.org/10.1007/BF00651077