Sentence examples for order spectra from inspiring English sources

Time varying higher order spectra (TVHOS) are designed for non-Gaussian non-stationary signal processing.

Some of these events can be recovered by examining higher order spectra but most pile-up events will have "migrated" out of the standard grade set.

The effect is most likely seen in first order spectra when observing bright continuum sources such as those found in the Galactic bulge.

Finally, the vibration features of gear faults can be clearly exposed by the envelope order spectra.

This can capture both linear and nonlinear serial dependence while avoiding the drawbacks of the conventional spectrum, which cannot capture nonlinear serial dependence, and higher order spectra (e.g., bispectrum), which requires the existence of restrictive moment conditions.

From Figure 1 one can see that S0 and S5 are useless for detecting 1st-order photons, although they may be useful for collecting higher order spectra in some cases.

An overlapping of the first order and second order spectrum is then observed.

9.29 The 1st order spectrum for an 80 ksec observation of the AGN NGC5548.

Note that the 6.7 Å lines are better resolved in the high order spectrum.

The envelope order spectrum is used for bearing fault identification.

Figure 9.29: This figure shows the extracted 1st order spectrum for an 80 ksec observation of the AGN NGC5548.