Since our approach allows for the finetuning of the signal noise decomposition by the FDR we scan a large range of FDRs and evaluate the obtained solutions in terms of recall (true-positive rate) and precision (ratio of true positives to all positively classified).
Simulations are conducted to obtain solutions in terms of streamlines, isotherms, local entropy generation contours, total entropy generation, Bejan number for various ranges of the magnetic force parameter and Rayleigh number in a nongravitational field.
Simulations have been done to obtain solutions in terms of isotherms, streamfunction and entropy generation maps (Sθ and Sψ) for various ranges of modified Darcy number (Da), Prandtl number (Pr) at modified Rayleigh number, Ra = 106.
As can be seen, parameter setting 1 obtained better solution in terms of solution time with the value of 312 mm since it has lesser fitness value and the value of (n) that is assigned to this parameter setting is lesser.
The advantage of using Jacobi polynomials for solving differential equations is obtaining the solution in terms of the Jacobi parameters α and β (see [24 27]).
Finally, a conclusion is drawn in Section 5. Due to obtaining the solution in terms of the Jacobi parameters α and β, the use of Jacobi polynomials for solving differential equations has gained increasing popularity in recent years (see, [32, 33]).
Once the adhesive model parameters obtained, they have been used to virtually study a prototype of the heat exchanger to obtain a suitable solution in terms of thermo-mechanical strength and energetic efficiency.
In Section 3, we prove a sufficient condition and we obtain the explicit solution in terms of and.
In order to obtain the optimum solution in terms of Pareto set, a genetic algorithm approach the NSGA-II is adopted.
A semi-infinite elastic solid subjected to line loading is considered with higher order boundary conditions is utilized to obtain a general solution in terms of Fourier integral transforms for a symmetrical line loading with prescribed normal tractions.
