Sentence examples for density of pressure from inspiring English sources

Exact(2)

Description of the turbulent pressure field is based on the Corcos formulation for cross spectral density of pressure fluctuations.

The cross spectral density of pressure fluctuations in the turbulent pressure field is described using the Corcos formulation.

Similar(57)

In addition, the mean and root mean square (RMS) values, the power spectra of the pressure fluctuations on the prism surface, the integral forces (lift and drag forces) and probability densities of pressure fluctuations are presented.

The simulations and experiments are compared through power spectral density distributions of pressure fluctuations in the bed and air plenum.

An amplitude division method based on the Gaussian distribution and the Kolmogorov Smirnov test was developed to divide the structure density distribution of pressure signals into three characteristic regions linked to: I. fine-scale structures, II.

The Z directions are divided into grid number of N H which represents the discrete point density of formation pressure along the vertical well depth.

A numerical approach is proposed to obtain the total root mean square displacements of an open curved thin structure in terms of the cross spectral density of random pressure fields.

The argument is directly analogous to the one applied in the previous section to waves on shallow water and, indeed, the diagrams in Figure 6 can serve to illustrate the argument here too, if they are regarded as plots of gas density (or else of pressure or temperature, which go hand in hand with density in adiabatic flow) versus position.

With the winged core, the turbulence structure characteristics inside the hydrocyclone, including time-averaged pressure, pressure fluctuation, relative pressure fluctuation characteristics, and distribution characteristics of the probability density of the turbulence pressure, were all positively controlled.

Primarily, solving an ordinary differential equation, the Hubble parameter has been reconstructed, and this has led to the reconstruction of the density and pressure of the said dark energy candidate.

The aerodynamic component of the excitation is applied on the basis of Corcos model where the power spectral density of the wall pressure is determined experimentally.

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