Laminar hydromagnetic thermal boundary layer in fluctuating flow past a limiting surface with variable suction

Details Laminar hydromagnetic thermal boundary layer in fluctuating flow past a limiting surface with variable suction Laminar hydromagnetic thermal boundary layer in fluctuating flow past a limiting surface with variable suction

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..74..265k&link_type=abstract

Astrophysics and Space Science, vol. 74, no. 2, Feb. 1981, p. 265-272. Research supported by the Alexander S. Onassis Foundation

Astronomy and Astrophysics

Astrophysics

Laminar Boundary Layer, Magnetohydrodynamic Flow, Porous Walls, Stellar Atmospheres, Suction, Thermal Boundary Layer, Unsteady Flow, Astronomical Models, Incompressible Flow, Prandtl Number, Thermodynamic Properties, Variations, Viscous Flow

Scientific paper

An analysis of the temperature field in the case of the two-dimensional hydromagnetic flow of a viscous incompressible and electrically conducting fluid, (e.g., of a stellar atmosphere), past a porous, infinite, limiting surface in the presence of a transverse magnetic field, is considered when (1) the free stream velocity oscillates in time about a constant mean; (2) the suction velocity normal to the limiting surface oscillates in magnitude but not in direction about a non-zero mean; (3) there is no heat transfer between the fluid and the wall, approximate solution is obtained of the energy equation and expressions given for the temperature field and for the temperature at the limiting surface, when the magnetic Prandtl number = 1 and magnetic parameter is less than 1.

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