lomb_scargle (pyleoclim.utils.spectral.lomb_scargle)

pyleoclim.utils.spectral.lomb_scargle(ys, ts, freq=None, freq_method='lomb_scargle', freq_kwargs=None, n50=3, window='hann', detrend=None, sg_kwargs=None, gaussianize=False, standardize=False, average='mean')[source]

Return the computed periodogram using lomb-scargle algorithm

Uses the lombscargle implementation from scipy.signal: https://scipy.github.io/devdocs/generated/scipy.signal.lombscargle.html#scipy.signal.lombscargle

Parameters
  • ys (array) – a time series

  • ts (array) – time axis of the time series

  • freq (str or array) – vector of frequency. If string, uses the following method:

  • freq_method (str) –

    Method to generate the frequency vector if not set directly. The following options are avialable:
    • log

    • lomb_scargle (default)

    • welch

    • scale

    • nfft

    See utils.wavelet.make_freq_vector for details

  • freq_kwargs (dict) – Arguments for the method chosen in freq_method. See specific functions in utils.wavelet for details By default, uses dt=median(ts), ofac=4 and hifac=1 for Lomb-Scargle

  • n50 (int) – The number of 50% overlapping segment to apply

  • window (str or tuple) –

    Desired window to use. Possible values:
    • boxcar

    • triang

    • blackman

    • hamming

    • hann (default)

    • bartlett

    • flattop

    • parzen

    • bohman

    • blackmanharris

    • nuttail

    • barthann

    • kaiser (needs beta)

    • gaussian (needs standard deviation)

    • general_gaussian (needs power, width)

    • slepian (needs width)

    • dpss (needs normalized half-bandwidth)

    • chebwin (needs attenuation)

    • exponential (needs decay scale)

    • tukey (needs taper fraction)

    If the window requires no parameters, then window can be a string. If the window requires parameters, then window must be a tuple with the first argument the string name of the window, and the next arguments the needed parameters. If window is a floating point number, it is interpreted as the beta parameter of the kaiser window.

    detrendstr
    If None, no detrending is applied. Available detrending methods:
    • None - no detrending will be applied (default);

    • linear - a linear least-squares fit to ys is subtracted;

    • constant - the mean of ys is subtracted

    • savitzy-golay - ys is filtered using the Savitzky-Golay filters and the resulting filtered series is subtracted from y.

    • emd - Empirical mode decomposition

    sg_kwargsdict

    The parameters for the Savitzky-Golay filters. see pyleoclim.utils.filter.savitzy_golay for details.

    gaussianizebool

    If True, gaussianizes the timeseries

    standardizebool

    If True, standardizes the timeseriesprep_args : dict

    average{‘mean’,’median’}

    Method to use when averaging periodograms. Defaults to ‘mean’.

Returns

res_dict – the result dictionary, including - freq (array): the frequency vector - psd (array): the spectral density vector

Return type

dict

See also

pyleoclim.utils.spectral.periodogram

Estimate power spectral density using a periodogram

pyleoclim.utils.spectral.mtm

Retuns spectral density using a multi-taper method

pyleoclim.utils.spectral.welch

Returns power spectral density using the Welch method

pyleoclim.utils.spectral.wwz_psd

Return the psd of a timeseries using wwz method.

pyleoclim.utils.filter.savitzy_golay

Filtering using Savitzy-Golay

pyleoclim.utils.tsutils.detrend

Detrending method

References

Lomb, N. R. (1976). Least-squares frequency analysis of unequally spaced data. Astrophysics and Space Science 39, 447-462.

Scargle, J. D. (1982). Studies in astronomical time series analysis. II. Statistical aspects of spectral analyis of unvenly spaced data. The Astrophysical Journal, 263(2), 835-853.

Scargle, J. D. (1982). Studies in astronomical time series analysis. II. Statistical aspects of spectral analyis of unvenly spaced data. The Astrophysical Journal, 263(2), 835-853.