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PPKE ITK PhD and MPhil Thesis Classes

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54<br />

2. MAPPING THE NUMERICAL SIMULATIONS OF PARTIAL<br />

DIFFERENTIAL EQUATIONS<br />

On the other h<strong>and</strong>, the development time of an optimized software solution is<br />

much shorter than designing a reconfigurable architecture [56][57], however, the<br />

computational efficiency is smaller in terms of area <strong>and</strong> power. Namely on FPGAs<br />

we can make a more specific structure for the CFD with better performance in<br />

terms of the area <strong>and</strong> dissipation with a variable accuracy considering to use it<br />

in real life applications.<br />

2.3.2 Fluid Flows<br />

A wide range of industrial processes <strong>and</strong> scientific phenomena involve gas or fluids<br />

flows over complex obstacles. In engineering applications the temporal evolution<br />

of non-ideal, compressible fluids is quite often modeled by Navier-Stokes [58, 59]<br />

equations. It is based on the fundamental laws of mass-, momentum- <strong>and</strong> energy<br />

conservation, extended by the dissipative effects of viscosity, diffusion <strong>and</strong> heat<br />

conduction. By neglecting all the above non-ideal processes, <strong>and</strong> assuming adiabatic<br />

variations, we obtain the Euler equations [60, 61], describing the dynamics<br />

of dissipation-free, inviscid, compressible fluids. The equations, a coupled set of<br />

nonlinear hyperbolic partial differential equations, in conservative form expressed<br />

as<br />

∂ (ρv)<br />

∂t<br />

∂E<br />

∂t<br />

∂ρ<br />

∂t<br />

+ ∇ · (ρv) = 0 (2.2)<br />

)<br />

+ ∇ ·<br />

(ρvv + Îp = 0 (2.3)<br />

+ ∇ · ((E + p)v) = 0, (2.4)<br />

where t denotes time, ∇ is the Nabla operator, ρ is the density, u, v are the x-<br />

<strong>and</strong> y-components of velocity vector v, respectively, p is the pressure of the fluid,<br />

Î is the identity matrix, <strong>and</strong> E is the total energy density defined as<br />

E =<br />

p<br />

γ − 1 + 1 ρv · v, (2.5)<br />

2<br />

where γ is the ratio of specific heats. It is convenient to merge (2.2), (2.3) <strong>and</strong><br />

(2.4) into hyperbolic conservation law form in terms of U = [ρ, ρu, ρv, E] <strong>and</strong> the

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