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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 254 (1997), S. 159-172 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract At time t〈0, a steady stationary condition of a fully ionised gas exists in space, such that the velocity components, the induced magnetic field and a uniform temperature are given by (0,0,0),(0, 0,Ho) and Θ, respectively, in the rectangular coordinate (x,y,z). At t =0, a sudden increase of temperature is applied at z = 0. If the Eckert terms are neglected, an integral transform technique is employed to solve for the z–axis related transient flow (U,V,0),(Ho), and temperature Θ (z,t). For large applied magnetic field, Ho the flow is observed to exhibit disturbance modes some of which are oscilatory, and some streaming modes are seen accompanied by the expected decays. For a thermally perturbed plasma the flow is seen to be largely governed by conduction parameters if viscous terms are not neglected under the MHD approximations.
    Type of Medium: Electronic Resource
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  • 2
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The problem of magnetohydrodynamic free-convection flow, with radiative heat transfer in porour media subject to time-dependent suction of an incompressible and optically transparent medium has been solved making fairly realistic assumption. For a small-time-dependent perturbation of the fluid velocity and temperatures, the nonlinear problem is tackled by asymptotic approximation, giving solutions for steady-flow on which a first-order transient component is superimposed. The effect of heat radiation and free convection on the flow of the fluid is demonstrated analytically and quantitatively. The flow field is seen to be affected mainly by radiation and convection parameters, in addition to the porosity and magnetic factors.
    Type of Medium: Electronic Resource
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