Эротические рассказы

Vibroacoustic Simulation. Alexander PeifferЧитать онлайн книгу.

Vibroacoustic Simulation - Alexander Peiffer


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was only applied to input and output. Imagine a system that has many sources that have random nature. In the case of a car this could be the exhaust noise, the cooling ventilation, and the engine. The noise linked to the stroke movement will be correlated to the component that is transmitted via the muffler to exhaust, whereas the flow noise generated by the turbulent flow in the muffler is not correlated to the stroke harmonics. Thus, in practical vibroacoustic systems there is a mix of sources that are correlated to each other. Some are independent – thus uncorrelated – and some are a mix of both, as the discussed exhaust example.

      Equations (1.196) and (1.195) can only be used in case of fully correlated input because each summand in those equations will have a different phase or time delay for each set of input signals taken from the ensemble of possible input or for each separate test.

      Consider a set of N random input signals as given in Equation (1.195) or (1.196). For the description of the input we need the power spectral density or autocorrelation of all signals fn(t) given by

       bold-italic upper S Subscript f f comma n n Baseline equals upper E left-bracket bold-italic upper F Subscript n Superscript asterisk Baseline left-parenthesis omega right-parenthesis bold-italic upper F Subscript n Baseline left-parenthesis omega right-parenthesis right-bracket (1.199)

      Here the index ff denotes that only the input is considered, and nn that it is the autocorrelation of the nth input. In addition the cross correlation between the input signals is given by:

       bold-italic upper S Subscript f f comma m n Baseline equals upper E left-bracket bold-italic upper F Subscript m Superscript asterisk Baseline left-parenthesis omega right-parenthesis bold-italic upper F Subscript n Baseline left-parenthesis omega right-parenthesis right-bracket (1.200)

      This expression is called the cross spectral density matrix that looks in large form

       Start 1 By 1 Matrix 1st Row bold-italic upper S Subscript f f Baseline EndMatrix equals Start 5 By 5 Matrix 1st Row 1st Column bold-italic upper S Subscript f f comma 11 Baseline left-parenthesis omega right-parenthesis 2nd Column midline-horizontal-ellipsis 3rd Column bold-italic upper S Subscript f f comma 1 n Baseline left-parenthesis omega right-parenthesis 4th Column midline-horizontal-ellipsis 5th Column bold-italic upper S Subscript f f comma 1 upper N Baseline 2nd Row 1st Column vertical-ellipsis 2nd Column down-right-diagonal-ellipsis 3rd Column vertical-ellipsis 4th Column down-right-diagonal-ellipsis 5th Column vertical-ellipsis 3rd Row 1st Column bold-italic upper S Subscript f f comma m Baseline 1 Baseline left-parenthesis omega right-parenthesis 2nd Column midline-horizontal-ellipsis 3rd Column bold-italic upper S Subscript f f comma m n Baseline left-parenthesis omega right-parenthesis 4th Column midline-horizontal-ellipsis 5th Column bold-italic upper S Subscript f f comma m upper N Baseline 4th Row 1st Column vertical-ellipsis 2nd Column down-right-diagonal-ellipsis 3rd Column vertical-ellipsis 4th Column down-right-diagonal-ellipsis 5th Column vertical-ellipsis 5th Row 1st Column bold-italic upper S Subscript f f comma upper N Baseline 1 Baseline left-parenthesis omega right-parenthesis 2nd Column midline-horizontal-ellipsis 3rd Column bold-italic upper S Subscript f f comma upper N n Baseline left-parenthesis omega right-parenthesis 4th Column midline-horizontal-ellipsis 5th Column bold-italic upper S Subscript f f comma upper N upper N EndMatrix (1.201)

      This is a hermitian matrix due to the symmetry relationship of cross spectra also following from the expected value of each spectral product

       bold-italic upper S Subscript f f comma n m Baseline equals upper E left-bracket bold-italic upper F Subscript n Superscript asterisk Baseline left-parenthesis omega right-parenthesis bold-italic upper F Subscript m Baseline left-parenthesis omega right-parenthesis right-bracket equals upper E left-bracket bold-italic upper F Subscript n Baseline left-parenthesis omega right-parenthesis bold-italic upper F Subscript m Superscript asterisk Baseline left-parenthesis omega right-parenthesis right-bracket Superscript asterisk Baseline equals bold-italic upper S Subscript f f comma m n Superscript asterisk (1.202)

      For further considerations it is helpful to write the cross spectral matrix using the input spectra in vector form. Because of the matrix multiplication notation – row times column – the cross spectral density matrix can be written as

       Start 1 By 1 Matrix 1st Row bold-italic upper S Subscript f f Baseline EndMatrix equals upper E left-bracket Start 4 By 1 Matrix 1st Row bold-italic upper F 1 Superscript asterisk Baseline left-parenthesis omega right-parenthesis 2nd Row bold-italic upper F 2 Superscript asterisk Baseline left-parenthesis omega right-parenthesis 3rd Row vertical-ellipsis 4th Row bold-italic upper F Subscript upper N Superscript asterisk Baseline left-parenthesis omega right-parenthesis EndMatrix Start 1 By 4 Matrix 1st Row 1st Column bold-italic upper F 1 left-parenthesis omega right-parenthesis 2nd Column bold-italic upper F 2 left-parenthesis omega right-parenthesis 3rd Column reverse-solidus hdots 4th Column bold-italic upper F Subscript upper N Baseline left-parenthesis omega right-parenthesis EndMatrix right-bracket equals upper E left-bracket Start 1 By 1 Matrix 1st Row bold-italic upper F EndMatrix Superscript asterisk Baseline Start 1 By 1 Matrix 1st Row bold-italic upper F EndMatrix Superscript upper T Baseline right-bracket (1.203)

       Start 1 By 1 Matrix 1st Row bold-italic upper S Subscript f f EndMatrix Superscript asterisk Baseline equals upper E left-bracket Start 4 By 1 Matrix 1st Row bold-italic upper F 1 left-parenthesis omega right-parenthesis 2nd Row bold-italic upper F 2 left-parenthesis omega right-parenthesis 3rd Row vertical-ellipsis 4th Row bold-italic upper F Subscript upper N Baseline left-parenthesis omega right-parenthesis EndMatrix Start 1 By 4 Matrix 1st Row 1st Column bold-italic upper F 1 Superscript asterisk Baseline left-parenthesis omega right-parenthesis comma 2nd Column bold-italic upper F 2 Superscript asterisk Baseline left-parenthesis omega right-parenthesis comma 3rd Column reverse-solidus hdots comma 4th Column bold-italic upper F Subscript upper N Superscript asterisk Baseline left-parenthesis omega right-parenthesis EndMatrix right-bracket equals upper E left-bracket Start 1 By 1 Matrix 1st Row bold-italic upper F EndMatrix Start 1 By 1 Matrix 1st Row bold-italic upper F EndMatrix Superscript upper H Baseline right-bracket (1.204)

      It is helpful to understand how the matrix coefficients look for the following extreme cases:

       Fully uncorrelated signals

       Fully correlated signals.

      The hermitian operator ⋅H is used, which combines the operations of complex conjugation and transposition.

      1.7.1.1 Fully Uncorrelated Signals – Rain on the Roof Excitation

      Fully uncorrelated input signals mean that the cross correlation is zero. A model of this is the “rain-on-the-roof” excitation because each drop falls fully independent from its brother drops on the roof. This means that the cross correlation matrix has only diagonal components. All off-diagonal components are zero.

      1.7.1.2 Fully Correlated Signals

      In this case the signals are correlated and have a clear phase relationship to a reference. Thus, all signals are linearly dependent to this reference. So every column of the cross spectral matrix can by derived by a linear combination of the other columns. So, we don’t need the full matrix and Equation (1.198)


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