3. Whitening a
This example requires LIGO.ORG credentials for data access.
Most data recorded from a gravitational-wave interferometer carry information across a wide band of frequencies, typically up to a few kiloHertz, but often it is the case that the low-frequency amplitude dwarfs that of the high-frequency content, making discerning high-frequency features difficult.
We employ a technique called ‘whitening’ to normalize the power at all frequencies so that excess power at any frequency is more obvious.
We demonstrate below with an auxiliary signal recording transmitted power in one of the interferometer arms, which recorded two large glitches with a frequency of around 5-50Hz.
from gwpy.timeseries import TimeSeries data = TimeSeries.get('H1:ASC-Y_TR_A_NSUM_OUT_DQ', 1123084671, 1123084703)
Now, we can
whiten the data to enhance the higher-frequency
white = data.whiten(4, 2)
plot both the original and whitened data
from gwpy.plot import Plot plot = Plot(data, white, separate=True, sharex=True) plot.axes.set_ylabel('Y-arm power [counts]', fontsize=16) plot.axes.set_ylabel('Whitened amplitude', fontsize=16) plot.show()
Here we see two large spikes that are completely undetected in the raw
TimeSeries, but are very obvious in the whitened data. We can also see
tapering effects at the boundaries as the whitening filter settles in,
meaning that the first and last ~second of data are corrupted and should
be discarded before further processing.