| System Identification Toolbox™ | ![]() |
h = idfrd(Response,Freq,Ts)
h = idfrd(Response,Freq,Ts,...
'CovarianceData',Covariance,'SpectrumData',Spec,...
'NoiseCovariance',Speccov)
h = idfrd(Response,Freq,Ts,...
'P1',V1,'PN',VN)
h = idfrd(mod)
h = idfrd(mod,Freqs)
h = idfrd(Response,Freq,Ts) constructs an idfrd object that stores the frequency response Response of a linear system at frequency values Freq. Ts is the sampling time interval. For a continuous-time system, set Ts=0.
h = idfrd(Response,Freq,Ts,...
'CovarianceData',Covariance,'SpectrumData',Spec,...
'NoiseCovariance',Speccov) also stores the
uncertainty of the response Covariance, the spectrum
of the additive disturbance (noise) Spec, and the
uncertainty of the noise Speccov.
h = idfrd(Response,Freq,Ts,...
'P1',V1,'PN',VN) constructs an idfrd object
that stores a frequency-response model with properties specified by
the idfrd model property-value pairs.
h = idfrd(mod) converts a System Identification Toolbox™ or Control System Toolbox linear model to frequency-response data at default frequencies, including the output noise spectra and their covariance. If the linear model has an input-to-output delay, this delay is converted to a phase lag.
h = idfrd(mod,Freqs) converts a System Identification Toolbox or Control System Toolbox linear model to frequency-response data at frequencies Freqs.
For a model
![]()
stores the transfer function estimate G
![]()
as well as the spectrum of the additive noise (
) at the output
![]()
where
is the estimated variance of e(t),
and T is the sampling interval.
Response is a 3-D array of dimension ny-by-nu-by-Nf,
with ny being the number of outputs, nu the
number of inputs, and Nf the number of frequencies
(that is, the length of Freqs). Response(ky,ku,kf) is
thus the complex-valued frequency response from input ku to
output ky at frequency
=Freqs(kf).
When defining the response of a SISO system, Response can
be given as a vector.
Freqs is a column vector of length Nf containing the frequencies of the response.
Ts is the sampling interval. T = 0 means a continuous-time model.
Covariance is a 5-D array containing the covariance of the frequency response. It has dimension ny-by-nu-by-Nf-by-2-by-2. The structure is such that Covariance(ky,ku,kf,:,:) is the 2-by-2 covariance matrix of the response Response(ky,ku,kf). The 1-1 element is the variance of the real part, the 2-2 element is the variance of the imaginary part, and the 1-2 and 2-1 elements are the covariance between the real and imaginary parts. squeeze(Covariance(ky,ku,kf,:,:)) thus gives the covariance matrix of the corresponding response.
The information about spectrum is optional. The format is as follows:
spec is a 3-D array of dimension ny-by-ny-by-Nf, such that spec(ky1,ky2,kf) is the cross spectrum between the noise at output ky1 and the noise at output ky2, at frequency Freqs(kf). When ky1 = ky2 the (power) spectrum of the noise at output ky1 is thus obtained. For a single-output model, spec can be given as a vector.
speccov is a 3-D array of dimension ny-by-ny-by-Nf, such that speccov(ky1,ky1,kf) is the variance of the corresponding power spectrum. Normally, no information is included about the covariance of the nondiagonal spectrum elements.
If only SpectrumData is to be packaged in the idfrd object, set Response = [].
idfrd can also be computed from a given model mod (defined as any idmodel object).
If the frequencies Freqs are not specified, a default choice is made based on the dynamics of the model mod.
If mod has InputDelay different from zero, these are appended as phase lags, and h will then have an InputDelay of 0.
The estimated covariances are computed using the Gauss approximation formula from the uncertainty information in mod. For models with complicated parameter dependencies, numerical differentiation is applied. The step sizes for the numerical derivatives are determined by nuderst.
Frequency responses for submodels can be obtained by the standard subreferencing, h = idfrd(m(2,3)). See idmodel. In particular, h = idfrf(m('measured')) gives an h that just contains the ResponseData (G) and no spectra. Also h = idfrd(m('noise')) gives an h that just contains SpectrumData.
The idfrd models can be graphed with bode, ffplot, and nyquist, which all accept mixtures of idmodel and idfrd models as arguments. Note that spa, spafdr, and etfe return their estimation results as idfrd objects.
ResponseData: 3-D array of the complex-valued frequency response as described above. For SISO systems use Response(1,1,:) to obtain a vector of the response data.
Frequency: Column vector containing the frequencies at which the responses are defined.
CovarianceData: 5-D array of the covariance matrices of the response data as described above.
SpectrumData: 3-D array containing power spectra and cross spectra of the output disturbances (noise) of the system.
NoiseCovariance: 3-D array containing the variances of the power spectra, as explained above.
Units: Unit of the frequency vector. Can assume the values 'rad/s' and 'Hz'.
Ts: Scalar denoting the sampling interval of the model whose frequency response is stored. 'Ts' = 0 means a continuous-time model.
Name: An optional name for the object.
InputName: String or cell array containing the names of the input channels. It has as many entries as there are input channels.
OutputName: Correspondingly for the output channels.
InputUnit: Units in which the input channels are measured. It has the same format as 'InputName'.
OutputUnit: Correspondingly for the output channels.
InputDelay: Row vector of length equal to the number of input channels. Contains the delays from the input channels. These should thus be appended as phase lags when the response is calculated. This is done automatically by freqresp, bode, ffplot, and nyquist. Note that if the idfrd is calculated from an idmodel, possible input delays in that model are converted to phase lags, and the InputDelay of the idfrd model is set to zero.
Notes: An arbitrary field to store extra information and notes about the object.
UserData: An arbitrary field for any possible use.
EstimationInfo: Structure that contains information about the estimation process that is behind the frequency data. It contains the following fields (see also the reference page for EstimationInfo).
Status: Gives the status of the model, for example, 'Not estimated'.
Method: The identification routine that created the model.
WindowSize: If the model was estimated by spa, spafdr, or etfe, the size of window (input argument M, the resolution parameter) that was used. This is scalar or a vector.
DataName: Name of the data set from which the model was estimated.
DataLength: Length of this data set.
Note that you can set or retrieve all properties either with the set and get commands or by subscripts. Autofill applies to all properties and values, and these are case insensitive:
h.ts = 0 loglog(h.fre,squeeze(h.spe(2,2,:)))
For a complete list of property values, use get(m). To see possible value assignments, use set(m). See also idprops idfrd.
The different channels of the idfrd are retrieved by subreferencing.
h(outputs,inputs)
h(2,3) thus contains the response data from input channel 3 to output channel 2, and, if applicable, the output spectrum data for output channel 2. The channels can also be referred to by their names, as in h('power',{'voltage', 'speed'}).
h('m')
contains the information for measured inputs only, that is, just ResponseData, while
h('n')
('n' for 'noise') just contains SpectrumData.
Adding input channels,
h = [h1,h2,...,hN]
creates an idfrd model h, with ResponseData containing all the input channels in h1,...,hN. The output channels of hk must be the same, as well as the frequency vectors. SpectrumData is ignored.
Adding output channels,
h = [h1;h2;... ;hN]
creates an idfrd model h with ResponseData containing all the output channels in h1, h2,...,hN. The input channels of hk must all be the same, as well as the frequency vectors. SpectrumData is also appended for the new outputs. The cross spectrum between output channels is then set to zero.
You can convert an idfrd object to a frequency-domain iddata object by
Data = iddata(Idfrdmodel)
See iddata.
Compare the results from spectral analysis and an ARMAX model.
m = armax(z,[2 2 2 1]);
g = spa(z)
g = spafdr(z,[],{0,10})
bode(g,m)
Compute separate idfrd models, one containing the frequency function and the other the noise spectrum.
g = idfrd(m('m'))
phi = idfrd(m('n'))
| bode | |
| etfe | |
| ffplot | |
| freqresp | |
| nyquist | |
| spa | |
| spafdr |
![]() | idfilt | idgrey | ![]() |
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