Radiation and Buoyancy Effects on MHD Stagnation Point Flow of Micropolar Fluids due to a Porous Stretching Sheet

Radiation and Buoyancy Effects on MHD Flow of Micropolar Fluids

Authors

  • Hassan Waqas Department of Mathematics, Government College University Faisalabad (Layyah Campus), Pakistan
  • Sajjad Hussain Department of Mathematics, Government College University Faisalabad (Layyah Campus), Pakistan
  • Shamila Khalid Department of Mathematics, Government College University Faisalabad (Layyah Campus), Pakistan

Keywords:

Micropolar fluids, Buoyancy effect, radiation, stretching sheet, similarity function

Abstract

Computational investigation for buoyancy and radiation effects on the magneto hydrodynamics stagnation point flow of micropolar fluids has been made to study the kinematics and temperature distribution under the influence of virtual parameter of physical importance. The similarity functions have been used to obtain the ordinary differential equations for non-linear partial differential model of the problem. The results have been computed by Mathematica software and presented the graphs of microrotation, temperature and velocity.

References

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Published

2021-04-29

How to Cite

Waqas, H. ., Hussain, S. ., & Khalid, S. . (2021). Radiation and Buoyancy Effects on MHD Stagnation Point Flow of Micropolar Fluids due to a Porous Stretching Sheet: Radiation and Buoyancy Effects on MHD Flow of Micropolar Fluids. Proceedings of the Pakistan Academy of Sciences: A. Physical and Computational Sciences, 54(2), 157–165. Retrieved from http://ppaspk.org/index.php/PPAS-A/article/view/245

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