Abstract
The flow equations of non-Newtonian EMFD flows are formulated in terms of stream function and magnetic flux function as a independent variable. The exact analytical solution of physical importance is obtained for orthogonal and radial flows.
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Barron, R. M., Chandna, O. P., and Prabhaharan, K.: 1984,Appl. Sci. Res. 41, 3.
Kaloni, P. N. and Siddiqui, A. M.: 1983,Int. J. Engg. Sci.
Martin, M. H.: 1971,Arch. Rat. Mech. Anal. 41, 266.
Rivlin, R. S. and Ericksen, J. L.: 1955,J. Rat. Mech. Anal. 4, 323.
Singh, H. P. and Tripathi, D. D.: 1990,Mech. Res. Comm. (accepted for publication).
Singh, H. P., Tripathi, D. D., and Mishra, R. B.: 1987a,Astrophys. Space Sci. 138, 315.
Singh, H. P., Tripathi, D. D., and Mishra, R. B.: 1987b,Astrophys. Space Sci. 139, 413.
Singh, H. P., Tripathi, D. D., and Mishra, R. B.: 1988,Astrophys. Space. Sci. 141, 415.
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Tripathi, D.D. Hodograph transformation in non-Newtonian EMFD flows. Astrophys Space Sci 174, 229–234 (1990). https://doi.org/10.1007/BF00642509
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DOI: https://doi.org/10.1007/BF00642509