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1. |
Non linear waves in two dimensional keplerian flows |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 38,
Issue 2,
1987,
Page 69-104
E. Siregar,
J. Léorat,
J.P. Poyet,
A. Pouquet,
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摘要:
Accretion discs in astrophysics are fundamental for converting gravitational binding energy into observed electromagnetic radiation. We study the behavior of waves in a two dimensional supersonic Keplerian flow inside a given gravitational potential. We present the effects of shearing and rotation on short waves, and the numerical study of the dynamical stability of such flows with respect to various perturbations. We show that a large class of dynamical effects, due to pressure and associated to short time scales, may be excited.
ISSN:0309-1929
DOI:10.1080/03091928708210106
出版商:Taylor & Francis Group
年代:1987
数据来源: Taylor
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2. |
On the exact shape of the horizontal profile of a topographically rectified tidal flow |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 38,
Issue 2,
1987,
Page 105-129
L.R. M. Maas,
J.T. F. Zimmerman,
N.M. Temme,
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摘要:
Starting from the nonlinear shallow water equations of a homogeneous rotating fluid we derive the equation describing the evolution of vorticity by a fluctuating bottom topography of small amplitude, using a multiple scale expansion in a small parameter, which is the topographic length scale relative to the tidal wave length. The exact response functions of residual vorticity for a sinusoidal bottom topography are compared with those obtained by a primitive perturbation series and by harmonic truncation, showing the former to be invalid for small topographic length scales and the latter to be only a fair approximation for vorticity produced by planetary vortex stretching. In deriving the exact shape of the horizontal residual velocity profile at a step-like break in the bottom topography, it is shown that the Lagrangian profile only exists in a strip having the width of the amplitude of the tidal excursion at both sides of the break, and that it vanishes outside that interval. Moreover, in the limit of small amplitude topography at least, it vanishes altogether for the generation mechanism by means of planetary vortex stretching. The Eulerian profile is shown to extend over twice the interval of the Lagrangian profile both for production by vortex stretching and by differential bottom friction. These finite intervals over which the residual velocity profiles exist for a step-like topography are not reproduced by harmonic truncation of the basic equation. This method gives exponentially decaying profiles, indicating spurious horizontal diffusion of vorticity. In terms of orders of magnitude, the method of harmonic truncation is reliable for residual velocity produced by vortex stretching but it overestimates the residual velocity produced by differential bottom friction by a factor 2.
ISSN:0309-1929
DOI:10.1080/03091928708210107
出版商:Taylor & Francis Group
年代:1987
数据来源: Taylor
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3. |
On material frame-indifference of turbulence closure models |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 38,
Issue 2,
1987,
Page 131-144
Goodarz Ahmadi,
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PDF (496KB)
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摘要:
The transformation of the second-order moment equation in turbulence under a change of frame is examined. The proper transformation of the apparent body force is included. It is shown that the second-order closure is consistent with the principle of material frame-indifference of continuum mechanics. The implications on second-order modeling are discussed.
ISSN:0309-1929
DOI:10.1080/03091928708210108
出版商:Taylor & Francis Group
年代:1987
数据来源: Taylor
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