aiaa#
Classes for importing AIAA Array Benchmarks.
These classes allow importing data from HDF5 files following the specifications of the AIAA microphone array methods benchmarking effort: https://www-docs.b-tu.de/fg-akustik/public/veroeffentlichungen/ArrayMethodsFileFormatsR2P4Release.pdf .
The classes are derived from according Acoular classes so that they can be used directly within the framework.
Examples#
>>> micgeom = MicAIAABenchmark(file='some_benchmarkdata.h5')
>>> timedata = TimeSamplesAIAABenchmark(file='some_benchmarkdata.h5')
Container for AIAA benchmark data in *.h5 format. |
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Container for tacho data in *.h5 format. |
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Class to load the CSM that is stored in AIAA Benchmark HDF5 file. |
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Provides the geometric arrangement of microphones in the array. |
- class acoular.aiaa.aiaa.TimeSamplesAIAABenchmark#
Bases:
TimeSamplesContainer for AIAA benchmark data in *.h5 format.
This class loads measured data from h5 files in AIAA benchmark format and and provides information about this data. Objects of this class behave similar to
TimeSamplesobjects.- result(num=128)#
Generate blocks of time-domain data iteratively.
The
result()method is a Python generator that yields blocks of time-domain data of the specified size. Data is either read from an HDF5 file (iffileis set) or from a NumPy array (ifdatais directly provided).- Parameters:
- num
int, optional The size of each block to be yielded, representing the number of time-domain samples per block.
- num
- Yields:
numpy.ndarrayA 2D array of shape (
num,num_channels) representing a block of time-domain data. The last block may have fewer thannumsamples if the total number of samples is not a multiple ofnum.
- Raises:
OSErrorIf no samples are available (i.e.,
num_samplesis0).
Examples
Create a generator and access blocks of data:
>>> import numpy as np >>> from acoular.sources import TimeSamples >>> ts = TimeSamples(data=np.random.rand(1000, 4), sample_freq=51200) >>> generator = ts.result(num=256) >>> for block in generator: ... print(block.shape) (256, 4) (256, 4) (256, 4) (232, 4)
Note that the last block may have fewer that
numsamples.
- file#
Full path to the
.h5file containing time-domain data.
- num_channels#
Number of input channels in the time data, set automatically based on the
loaded dataorspecified array.
- num_samples#
Total number of time-domain samples, set automatically based on the
loaded dataorspecified array.
- data#
A 2D NumPy array containing the time-domain data, shape (
num_samples,num_channels).
- metadata#
Metadata loaded from the HDF5 file, if available.
- digest#
A unique identifier for the samples, based on its properties. (read-only)
- sample_freq#
Sampling frequency of the signal, defaults to 1.0
- class acoular.aiaa.aiaa.TriggerAIAABenchmark#
Bases:
TimeSamplesAIAABenchmarkContainer for tacho data in *.h5 format.
This class loads tacho data from h5 files as specified in “Microphone Array Benchmark b11: Rotating Point Sources” (https://doi.org/10.14279/depositonce-8460) and and provides information about this data.
- result(num=128)#
Generate blocks of time-domain data iteratively.
The
result()method is a Python generator that yields blocks of time-domain data of the specified size. Data is either read from an HDF5 file (iffileis set) or from a NumPy array (ifdatais directly provided).- Parameters:
- num
int, optional The size of each block to be yielded, representing the number of time-domain samples per block.
- num
- Yields:
numpy.ndarrayA 2D array of shape (
num,num_channels) representing a block of time-domain data. The last block may have fewer thannumsamples if the total number of samples is not a multiple ofnum.
- Raises:
OSErrorIf no samples are available (i.e.,
num_samplesis0).
Examples
Create a generator and access blocks of data:
>>> import numpy as np >>> from acoular.sources import TimeSamples >>> ts = TimeSamples(data=np.random.rand(1000, 4), sample_freq=51200) >>> generator = ts.result(num=256) >>> for block in generator: ... print(block.shape) (256, 4) (256, 4) (256, 4) (232, 4)
Note that the last block may have fewer that
numsamples.
- file#
Full path to the
.h5file containing time-domain data.
- num_channels#
Number of input channels in the time data, set automatically based on the
loaded dataorspecified array.
- num_samples#
Total number of time-domain samples, set automatically based on the
loaded dataorspecified array.
- data#
A 2D NumPy array containing the time-domain data, shape (
num_samples,num_channels).
- metadata#
Metadata loaded from the HDF5 file, if available.
- digest#
A unique identifier for the samples, based on its properties. (read-only)
- sample_freq#
Sampling frequency of the signal, defaults to 1.0
- class acoular.aiaa.aiaa.CsmAIAABenchmark#
Bases:
PowerSpectraImportClass to load the CSM that is stored in AIAA Benchmark HDF5 file.
- file#
Full name of the .h5 file with data
- basename#
Basename of the .h5 file with data, is set automatically.
- num_channels#
number of channels
- digest#
A unique identifier for the CSM importer, based on its properties. (read-only)
- fftfreq()#
Return the Discrete Fourier Transform sample frequencies.
- Returns:
- ndarray
Array of length block_size/2+1 containing the sample frequencies.
- calc_csm()#
Calculate the CSM for the given source data.
This method computes the CSM by performing a block-wise Fast Fourier Transform (FFT) on the source data, applying a window function, and averaging the results. Only the upper triangular part of the matrix is computed for efficiency, and the lower triangular part is constructed via transposition and complex conjugation.
- Returns:
numpy.ndarrayThe computed cross spectral matrix as an array of shape
(n, m, m)of complex values fornfrequencies andmchannels as innum_channels.
Examples
>>> import numpy as np >>> from acoular import TimeSamples >>> from acoular.spectra import PowerSpectra >>> >>> data = np.random.rand(1000, 4) >>> ts = TimeSamples(data=data, sample_freq=51200) >>> print(ts.num_channels, ts.num_samples, ts.sample_freq) 4 1000 51200.0 >>> ps = PowerSpectra(source=ts, block_size=128, window='Blackman') >>> ps.csm.shape (65, 4, 4)
- calc_ev()#
Calculate eigenvalues and eigenvectors of the CSM for each frequency.
The eigenvalues represent the spectral power, and the eigenvectors correspond to the principal components of the matrix. This calculation is performed for all frequency slices of the CSM.
- Returns:
tupleofnumpy.ndarray- A tuple containing:
eva(numpy.ndarray): Eigenvalues as a 2D array of shape(n, m), wherenis the number of frequencies andmis the number of channels. The datatype depends on the precision.eve(numpy.ndarray): Eigenvectors as a 3D array of shape(n, m, m). The datatype is consistent with the precision of the input data.
Notes
The precision of the eigenvalues is determined by
precision('float64'forcomplex128precision and'float32'forcomplex64precision).This method assumes the CSM is already computed and accessible via
csm.
Examples
>>> import numpy as np >>> from acoular import TimeSamples >>> from acoular.spectra import PowerSpectra >>> >>> data = np.random.rand(1000, 4) >>> ts = TimeSamples(data=data, sample_freq=51200) >>> ps = PowerSpectra(source=ts, block_size=128, window='Hanning') >>> eva, eve = ps.calc_ev() >>> print(eva.shape, eve.shape) (65, 4) (65, 4, 4)
- calc_eva()#
Calculate eigenvalues of the CSM.
This method computes and returns the eigenvalues of the CSM for all frequency slices.
- Returns:
numpy.ndarrayA 2D array of shape
(n, m)containing the eigenvalues fornfrequencies andmchannels. The datatype depends onprecision('float64'forcomplex128precision and'float32'forcomplex64precision).
Notes
This method internally calls
calc_ev()and extracts only the eigenvalues.
- calc_eve()#
Calculate eigenvectors of the Cross Spectral Matrix (CSM).
This method computes and returns the eigenvectors of the CSM for all frequency slices.
- Returns:
numpy.ndarrayA 3D array of shape
(n, m, m)containing the eigenvectors fornfrequencies andmchannels. Each sliceeve[f]represents an(m, m)matrix of eigenvectors for frequencyf. The datatype matches theprecisionof the CSM (complex128orcomplex64).
Notes
This method internally calls
calc_ev()and extracts only the eigenvectors.
- synthetic_ev(freq, num=0)#
Retrieve synthetic eigenvalues for a specified frequency or frequency range.
This method calculates the eigenvalues of the CSM for a single frequency or a synthetic frequency range. If
numis set to0, it retrieves the eigenvalues at the exact frequency. Otherwise, it averages eigenvalues across a range determined byfreqandnum.- Parameters:
- freq
float The target frequency for which the eigenvalues are calculated. This is the center frequency for synthetic averaging.
- num
int, optional The number of subdivisions in the logarithmic frequency space around the center frequency
freq.0(default): Only the eigenvalues for the exact frequency line are returned.Non-zero:
num
frequency band width
0
single frequency line
1
octave band
3
third-octave band
n
1/n-octave band
- freq
- Returns:
numpy.ndarrayAn array of eigenvalues. If
num == 0, the eigenvalues for the single frequency are returned. Fornum > 0, a summed array of eigenvalues across the synthetic frequency range is returned.
Examples
>>> import numpy as np >>> from acoular import TimeSamples >>> from acoular.spectra import PowerSpectra >>> np.random.seed(0) >>> >>> data = np.random.rand(1000, 4) >>> ts = TimeSamples(data=data, sample_freq=51200) >>> ps = PowerSpectra(source=ts, block_size=128, window='Hamming') >>> ps.synthetic_ev(freq=5000, num=5) array([0.00048803, 0.0010141 , 0.00234248, 0.00457097]) >>> ps.synthetic_ev(freq=5000) array([0.00022468, 0.0004589 , 0.00088059, 0.00245989])
- csm#
The cross-spectral matrix stored in an array of shape
(n, m, m)of complex fornfrequencies andmchannels.
- frequencies#
The frequencies included in the CSM in ascending order. Accepts list, array, or a single float value.
- source#
PowerSpectraImportdoes not consume time data; source is alwaysNone.
- sample_freq#
Sampling frequency of the signal. Default is
None
- block_size#
Block size for FFT, non-functional in this class.
- window#
Windowing method, non-functional in this class.
- overlap#
Overlap between blocks, non-functional in this class.
- cached#
Caching capability, always disabled.
- num_blocks#
Number of FFT blocks, always
None.
- ind_low#
Index of lowest frequency line to compute. Default is
1. Only used by objects that fetch the CSM. PowerSpectra computes every frequency line.
- ind_high#
Index of highest frequency line to compute. Default is
-1(last possible line for defaultblock_size).
- freq_range#
2-element array with the lowest and highest frequency. If the higher frequency is larger than the max frequency, the max frequency will be the upper bound.
- eva#
The eigenvalues of the CSM, stored as an array of shape
(n,)of floats fornfrequencies. (read-only)
- eve#
The eigenvectors of the cross spectral matrix, stored as an array of shape
(n, m, m)of floats fornfrequencies andmchannels as innum_channels. (read-only)
- precision#
Precision of the FFT, corresponding to NumPy dtypes. Default is
'complex128'.
- class acoular.aiaa.aiaa.MicAIAABenchmark#
Bases:
MicGeomProvides the geometric arrangement of microphones in the array.
In contrast to standard Acoular microphone geometries, the AIAA benchmark format includes the array geometry as metadata in the file containing the measurement data.
- file#
Name of the .h5-file from which to read the data.
- export_mpos(filename)#
Export the microphone positions to an XML file.
This method generates an XML file containing the positions of all valid microphones in the array. Each microphone is represented by a
<pos>element withName,x,y, andzattributes. The generated XML is formatted to match the structure required for importing into theMicGeomclass.- Parameters:
- filename
str The path to the file to which the microphone positions will be written. The file extension must be
.xml.
- filename
- Raises:
OSErrorIf the file cannot be written due to permissions issues or invalid file paths.
Notes
The file will be saved in UTF-8 encoding.
The
Nameattribute for each microphone is set as"Point {i+1}", whereiis the index of the microphone.This method only exports the positions of the valid microphones (those not listed in
invalid_channels).All coordinates (x, y, z) are exported in meters by default (see here).
- pos_total#
Array containing the
x, y, zpositions of all microphones, including invalid ones, shape(3,num_mics). This is set automatically whenfilechanges or explicitly by assigning an array of floats. All coordinates are in meters by default (see here).
- pos#
Array containing the
x, y, zpositions of valid microphones (i.e., excluding those ininvalid_channels), shape(3,num_mics). (read-only) All coordinates are in meters by default (see here).
- invalid_channels#
List of indices indicating microphones to be excluded from calculations and results. Default is
[].
- num_mics#
Number of valid microphones in the array. (read-only)
- center#
The geometric center of the array, calculated as the arithmetic mean of the positions of all valid microphones. (read-only)
- aperture#
The maximum distance between any two valid microphones in the array. (read-only)
- digest#
A unique identifier for the geometry, based on its properties. (read-only)