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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Zeitschrift für angewandte Mathematik und Physik 34 (1983), S. 867-885 
    ISSN: 1420-9039
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mathematics , Physics
    Description / Table of Contents: Résumé Cet article étudie l'écoulement d'un fluide de Newton visqueux oscillant avec une vitesse angulaireλ et une amplitudeV ∞ autour d'une sphère rigide, de rayona, tournant lentement sur elle-même à la vitesse angulaire ω. Siv est la viscosité d'écoulement, trois paramètres sont utilisés pour cette analyse: le nombre d ReynoldsR =V ∞ α/v les nombres de Taylorτ=a 2 w/v et σ=a 2 λ/v. On emploie une approximation asymptotique pourR etτ petits, σ quelconque. Dans la partie déterminante de l'approximation, la vitesse de rotation est celle d'un système à double roulement alors que les vitesses d'oscillation radiale et tangentielle rapellent les célèbres équations de Stokes (1851). Si l'approximation est d'ordreτ 2/R, la vitesse de rotation disparaît alors que les autres vitesses sont de nature non-oscillatoires et indépendantes deσ. Si l'approximation est d'ordreR, la vitesse de rotation est uniquement de nature oscillatoire tandis que les vitesses radiales et tangentielles ont des composantes à caractère stationaire auxquelles se superposent des composantes oscillatoires. Une étude quantitative révèle que ces composantes stationaires sont d'autant plus importantes queσ est petit.
    Notes: Summary In this paper the flow of a Newtonian viscous fluid, oscillating with angular velocityλ and amplitudeV ∞, past a rigid sphere of radiusa which is slowly rotated with angular velocity ω is studied. Denoting the kinematic viscosity of the fluid byv, three parameters are involved in the analysis, namely: the Reynolds numberR =V ∞ α/v and the Taylor numbersτ=a 2ω/v andσ=a 2 gl/v. Asymptotic approximation is employed assuming thatR andτ are small whileσ is arbitrary. In the leading approximation, the swell velocity represents a double roll system while the oscillatory radial and polar velocities are reminiscent of Stokes (1851) celebrated solutions. In the terms of orderτ 2/R approximation, the swell velocity is suppressed while the remaining two velocities are purely steady and independent ofσ. When the approximation is of orderR, the swell velocity is now purely oscillatory while the radial and polar velocities exhibit steady streaming components on which are superimposed oscillatory components. A quantitative study reveals that the steady streaming velocities are larger whenσ is small than when it is large.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    Zeitschrift für angewandte Mathematik und Physik 36 (1985), S. 767-774 
    ISSN: 1420-9039
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mathematics , Physics
    Description / Table of Contents: Zusammenfassung Es wird die Bewegung eines Fluids entlang einer heißen vertikalen Platte untersucht in Gegenwart eines außen angebrachten Magnetfeldes, im Falle daß die Strahlung wichtig ist. Obwohl die Geschwindigkeiten klein sind, werden in dieser Arbeit Kompressibilitätseffekte berücksichtigt, da bei Strahlungsproblemen hohe Temperaturen auftreten. Die Zähigkeitμ und der WärmeleitungskoeffizientK werden mit der Temperatur veränderlich angenommen, mitμ∼T n, und der Prandtl-ZahlPr=μc p/K konstant. Für den Strahlungsfluß wird eine allgemeine différentielle Form angenommen, und das asymptotische Problem, gültig in einigem Abstand von den Plattenenden, wird auf ein System von nichtlinearen gekoppelten gewöhnlichen Differentialgleichungen reduziert. Die Lösung des Problems wird quantitativ diskutiert.
    Notes: Summary Fluid motion generated by a long vertical hot plate in the presence of an externally applied magnetic field is investigated when radiative transfer is important. Even though the velocities involved are small, this paper takes compressibility into effect owing to the extreme heat encountered in radiation problems. Thus the viscosity (μ) and the thermal conductivity (K) are assumed to vary with the temperature (T). In this paper we takeμαT n while the Prandtl number (Pr) which is defined in terms of the specific heat at constant pressure (c p) byPr=μc p/K is constant. Assuming a general differential approximation for the radiative flux, the asymptotic problem, valid far away from the tips of the plate, is reduced to a set of nonlinear coupled ordinary differntial equations. Solution to this problem is discussed quantitatively.
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 192 (1992), S. 133-139 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The problem of unsteady flow of a relativistic radiating neutrino gas is studied by imposing a time-dependent perturbation on a basic flow. When the perturbation is small, the problem, which is ill-posed, is reduced to a well-posed spatial value problem for the transverse velocity and the temperature. Subsequently the axial velocity and number density may be obtained by straightforward integration with respect to time and imposition of the initial condition. The solution for the initial value problem is tackled by the Laplace transform technique and the results are discussed quantitatively.
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 192 (1992), S. 201-207 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The unsteady flow of a relativistic radiating neutrino gas is studied in a gravitational field. The curved body is assumed to be a vertical flat plate on which is imposed a time-dependent perturbation on a basic flow. For small perturbations, the ill-posed problem is reduced to a well-posed one and analytical solutions are developed.
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 195 (1992), S. 431-439 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The paper studies the hydromagnetic flow of a thermally-radiating binary mixture of an incompressible fluid. Both the Soret and Dufour effects are considered when the fluid is not chemically reacting. When the gas is optically thin the resultant system of ordinary differential equations could be solved in a closed form. Generally the problem is reduced to a set of integral equations which are tackled by perturbation and iteration. The problem is worthy of note in the re-entry problem.
    Type of Medium: Electronic Resource
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 195 (1992), S. 441-445 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The hydromagnetic flow in a vertical channel with heat and mass transfer is studied when chemical reaction is present. For the general integral equation for radiative flux and in the absence of the Dufour term, the problem is reduced to a set of coupled integral equations which are solved iteratively. The results are compared with the solutions obtained when chemical reaction is absent.
    Type of Medium: Electronic Resource
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  • 7
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 197 (1992), S. 61-76 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The paper studies the flow of a two-component hot plasma in a porous rotating sphere. Asymptotic solutions are derived for small rotation Reynolds number (Re). The overall analysis of the study shows that the temperature distribution of the gas inside the sphere has a minimum value, for the various values of the radiation parameterN 2 at a point where the radius of the solar sphere is 0.5r ⊙ (wherer 0 is the dimensional radius of the sphere). The general result of the studies are discussed quantitatively. The problem has a lot of application in the understanding of the interior of astrophysical bodies.
    Type of Medium: Electronic Resource
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  • 8
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 204 (1993), S. 87-96 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract In this paper, analytical MHD studies are made on the propagation of oscillatory waves in a semi-infinite plasma which is exposed to an applied magnetic field. The oscillatory wave is introduced into the plasma environment by temperature perturbation. The phase speeds of the resultant disturbance are discussed in terms Grashof, Prandtl, and Eckert numbers (free-convection parameters), Hall parameter, Alfvén parameter, and frequences. Expansion about small Eckert number is made to solve the very nonlinear coupled partial differential equations for the field variables. The appearance of steady streaming at all times in the first order expansion is mentioned.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 143 (1988), S. 225-232 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract This paper investigates transient effects on the flow of a thermally-radiating and electrically-conducting compressible gas in a rotating medium bounded by a vertical flat plate. The transience is provoked by a time-dependent perturbation on a constant plate temperature. The problem particularly focusses on an optically thick gas and a gas of arbitrary optical thickness when the difference between the wall and free-stream temperatures is small. Analytical results are possible only for limiting values of time and these results are discussed quatitatively. Indeed the assumption of small temperature difference is more appropriate for plates which are opaque than transparent.
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 189 (1992), S. 57-62 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract In this paper, the shock hodograph (polar) for a collisionless transverse shock has been developed in the plane of the flow deflection angle and total pressure jump. The sonic point on the hodograph lies closer to the characteristic than to the point of maximum flow deflection for an attached shock. This hodograph is particularly useful in the analysis of three shock confluences and refraction of shock waves at gas interfaces. The first analysis is fully described in this paper. It is observed that the third shock wave is forward facing. It is pertinent to note that the limited region of supersonic flow also restricts the occurrences of three shock interactions.
    Type of Medium: Electronic Resource
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