mth5.timeseries.spectre.spectrogram
Module contains a class that represents a spectrogram. i.e. A 2D time series of Fourier coefficients with axes time and the other frequency. The datasets are xarray/dataframe and are fundmentally multivariate.
Classes
Class to contain methods for STFT objects. |
Functions
|
Extracts a frequency band from xr.DataArray representing a spectrogram. |
Module Contents
- class mth5.timeseries.spectre.spectrogram.Spectrogram(dataset: xarray.Dataset | None = None)[source]
Bases:
objectClass to contain methods for STFT objects.
TODO: Add OLS Z-estimates – actually, these are properties of cross powers, not direct properties of spectrograms. TODO: Add Sims/Vozoff Z-estimates – actually, these are properties of cross powers as well. Note Coherence is similarly, a property of cross powers. There are in fact, very few features that we would derive from an unaveraged spectrogram. Pretty much everything except statistical moments comes from cross powers.
Development Notes: - The spectrogram class is fundamental to MT Processing, and normally appears during the STFT operation. - The extract_band method returns another Spectrogram, having the same time axis as the parent object, but only a slice of the frequency range. Both of these have in common that their frequency axes are uniformly spaced, delta-f, where delta-f is dictated by the time series sample rate and the FFT window lenght. - There is a sibling spectral-time-series container that should be considered. Call it for now, a FrequencyChunkedSpectrogram (or an AveragedSpectrogram). This is a container similar to spectrogram, but the frequencies are not uniformly spaced (instead, often logartihmically spaced), they are made from one or more (possibly multivariate) spectrograms, and a FrequencyBands object. The key difference is that in a FrequencyChunkedSpectrogram object has a non-uniform spaced the Frequency axis which was prescribed by a metadata object. Most features, as well as TFs have a FrequencyChunkedSpectrogram representation, where final TFs are just time-averaged a FrequencyChunkedSpectrograms.
TODO: consider factoring a simpler class that does not make the uniform frequency axis assumption. Spectrogram would extend this class and add the _frequency_increment property (taken from the differece in the first two values of the frequency axis), and num_harmoincs in band.
- property frequency_band: mt_metadata.common.band.Band[source]
returns a frequency band object representing the spectrograms band (assumes continuous)
- property frequency_increment[source]
returns the “delta f” of the frequency axis - assumes uniformly sampled in frequency domain
- num_harmonics_in_band(frequency_band: mt_metadata.common.band.Band, epsilon: float = 1e-07) int[source]
Returns the number of harmonics within the frequency band in the underlying dataset
- Parameters:
frequency_band
stft_obj
- Returns:
num_harmonics – The number of harmonics in the underlying dataset within the given frequency band.
- Return type:
int
- extract_band(frequency_band: mt_metadata.common.band.Band, channels: list | None = None, epsilon: float | None = None)[source]
Returns another instance of Spectrogram, with the frequency axis reduced to the input band.
- Parameters:
frequency_band
channels
- Returns:
spectrogram – Returns a Spectrogram object with only the extracted band for a dataset
- Return type:
aurora.time_series.spectrogram.Spectrogram
- cross_power_label(ch1: str, ch2: str, join_char: str = '_')[source]
joins channel names with join_char
- cross_powers(frequency_bands: mt_metadata.processing.aurora.frequency_bands.FrequencyBands, channel_pairs: List[Tuple[str, str]] | None = None)[source]
Compute cross powers between channel pairs for given frequency bands.
TODO: Add handling for case when band in frequency_bands is not contained in self.frequencies.
- Parameters:
frequency_bands (FrequencyBands) – The frequency bands to compute cross powers for. Each element of this iterable tells the lower and upper bounds of the cross-power calculation bands. These may become objects with information about tapers as ewwll.
channel_pairs (list of tuples, optional) – List of channel pairs to compute cross powers for. If None, all possible pairs will be used.
- Returns:
Dataset containing cross powers for all channel pairs. Each variable is named by the channel pair (e.g. ‘ex_hy’) and contains a 2D array with dimensions (frequency, time). All variables share common frequency and time coordinates.
- Return type:
xr.Dataset
- covariance_matrix(band_data: Spectrogram | None = None, method: str = 'numpy_cov') xarray.DataArray[source]
TODO: Add tests for this WIP Work-in-progress method Compute full covariance matrix for spectrogram data.
For complex-valued data, the result is a Hermitian matrix where: - diagonal elements are real-valued variances - off-diagonal element [i,j] is E[ch_i * conj(ch_j)] - off-diagonal element [j,i] is the complex conjugate of [i,j]
- Parameters:
band_data (Spectrogram, optional) – If provided, compute covariance for this data If None, use the full spectrogram
method (str) – Computation method. Currently only supports ‘numpy_cov’
- Returns:
Hermitian covariance matrix with proper channel labeling For channels i,j: matrix[i,j] = E[ch_i * conj(ch_j)]
- Return type:
xr.DataArray
- flatten(chunk_by: Literal['time', 'frequency'] = 'time') xarray.Dataset[source]
Reshape the 2D spectrogram into a 1D flattened xarray (time-chunked by default).
- Parameters:
chunk_by (Literal["time", "frequency"]) – Reshaping the 2D spectrogram can be done two ways, (basically “row-major”, or column-major). In xarray, but we either keep frequency constant and iterate over time, or keep time constant and iterate over frequency (in the inner loop).
- Returns:
xarray.Dataset (The dataset from the band spectrogram, stacked.)
Development Notes
The flattening used in tf calculation by default is opposite to here
dataset.stack(observation=(“frequency”, “time”))
However, for feature extraction, it may make sense to swap the order
xrds = band_spectrogram.dataset.stack(observation=(“time”, “frequency”))
This is like chunking into time windows and allows individual features to be computed on each time window – if desired.
Still need to split the time series though–Splitting to time would be a reshape by (last_freq_index-first_freq_index).
Using pure xarray this may not matter but if we drop down into numpy it could be useful.
- mth5.timeseries.spectre.spectrogram.extract_band(frequency_band: mt_metadata.common.band.Band, fft_obj: xarray.Dataset | xarray.DataArray, channels: list | None = None, epsilon: float = 1e-07) xarray.Dataset | xarray.DataArray[source]
Extracts a frequency band from xr.DataArray representing a spectrogram.
TODO: Update variable names.
- Development Notes:
Base dataset object should be a xr.DataArray (not xr.Dataset) - drop=True does not play nice with h5py and Dataset, results in a type error. File “stringsource”, line 2, in h5py.h5r.Reference.__reduce_cython__ TypeError: no default __reduce__ due to non-trivial __cinit__ However, it works OK with DataArray.
- Parameters:
frequency_band (mt_metadata.common.band.Band) – Specifies interval corresponding to a frequency band
fft_obj (xarray.core.dataset.Dataset) – Short-time-Fourier-transformed datat. Can be multichannel.
channels (list) – Channel names to extract.
epsilon (float) – Use this when you are worried about missing a frequency due to round off error. This is in general not needed if we use a df/2 pad around true harmonics.
- Returns:
extracted_band – The frequencies within the band passed into this function
- Return type:
xr.DataArray