Exact(6)
For every wind speed, free vibration test of section model is generally repeated several times in order to obtain more reliable parameter estimates.
We employ this scenario, more realistic than the simple smooth-wave test of Section 4.1.1, to measure the convergence order of the EL5 and MP5 methods.
It is validated in the subjective test of Section 5 that the spatial image width could be widened significantly and a better overall quality could be achieved compared to the BCC scheme without using the time difference cue.
We next test the EL5 scheme against a series of three-dimensional tests mostly based on the evolution of single, isolated neutron stars in general relativity (with the exception of grazing-collision test of Section 4.2.6).
Since the sources have low overlapping rate, we suppose that the observations detected by the thresholding test of Section "Weak-sparseness-based time frequency detection for source recovery (multisource selection)" mostly pertain to one signal source.
where A J # = ( A J H A J ) − 1 A J H is the Moore-Penrose pseudoinverse of A J. We propose to use the noise standard deviation estimate provided by the DATE to jointly denoise and separate the sources on the basis of the time frequency points selected by the statistical test of Section "Weak-sparseness-based time frequency detection for source recovery (multisource selection)".
Similar(54)
Classical music signals 1 3 that were used in the listening tests of Section 5.1 (and are used for the listening tests of this section as well) are part of this 1 minute testing dataset.
This paper presents an enhanced and more efficient procedure to identify rational functions and aerodynamic derivatives from wind tunnel tests of section models.
The system inferred all the road segments (some of which did not even exist in the base map of the tests of Section 7).
In Section "Simulation results", we apply the statistical tests of Section "Statistical tests for sparseness-based UBSS" to several standard UBSS methods[15, 16, 18, 26, 27] in the instantaneous mixture case.
In the interest of simplicity, the discussion is limited to special relativity, while the general-relativistic case, which is relevant for the neutron-star tests of Section 4.2, can be found in Appendix 1.
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