Spectrum plots =========================== Spectrum plots label their axes as F and Y. It defaults to a log-log plot the most common if not standard presentation in LIGO. To manually set the limits of the plot use ``--fmin`` and ``--fmax`` for the frequency axis and ``--ymin`` and ``--ymax`` for the Amplitude axis. If any are left blank they are set to the min or max of the data. If you prefer linear axes use the ``--nologf`` and ``--nology`` parameters. This can be useful to zoom in on peaks and lines in the spectrum. The spectrum presented is an average of multiple FFTs controled by ``--secpfft`` and ``--overlap``. ``--secpfft`` specifies the length of the FFT in seconds (not limited to powers of 2 or integers) and ``--overlap`` specifies a fractional overlap for the next FFT. For example a 1 second FFT of a 100 Hz channel with an overlap of 0.1 would generate the first FFT with samples 0-99 and the second FFT with samples 10-109. More overlap results in more averaging and a higher SNR. Longer FFTs result in better frequency resolution and less "frequency bleed". For example the following command line produces a fairly high frequency resolution plot of OAF-CAL_DARM from the 2014-02-14 lock at LLO: .. code-block:: sh gwpy-plot spectrum --chan L1:OAF-CAL_DARM_DQ --start 1107936067 --duration 120 --secpfft 10 .. image:: /../cli_examples/cli-sp-01.png :align: center :alt: Spectrum of OAF-CAL_DARM To zoom in on the lines between 500 and 700 Hz we could use the following: .. code-block:: sh gwpy-plot spectrum --chan L1:OAF-CAL_DARM_DQ --start 1107936067 --duration 120 \ --secpfft 10.000 --overlap 0.90 --nologf --fmin 500 --fmax 700 .. image:: /../cli_examples/cli-sp-02.png :align: center :alt: Zoom into spectrum of OAF-CAL_DARM Because the question such a plot could answer is exactly where are the lines, we use a linear frequency axis. Longer FFTs and a smaller frequency range would produce more resolution. The full help text for the Spectrum plot product is: .. code-block:: sh $ gwpy-plot spectrum --help usage: gwpy_ldvw spectrum [-h] [-v] [-s SILENT] --chan CHAN [CHAN ...] --start START [START ...] [--duration DURATION] [-c FRAMECACHE] [--highpass HIGHPASS] [--secpfft SECPFFT] [--overlap OVERLAP] [--nologf] [--fmin FMIN] [--fmax FMAX] [--nology] [--ymin YMIN] [--ymax YMAX] [-g GEOMETRY] [--interactive] [--title TITLE] [--suptitle SUPTITLE] [--xlabel XLABEL] [--ylabel YLABEL] [--out OUT] [--legend [LEGEND [LEGEND ...]]] [--nolegend] [--nogrid] optional arguments: -h, --help show this help message and exit -v, --verbose increase verbose output -s SILENT, --silent SILENT show only fatal errors --chan CHAN [CHAN ...] One or more channel names. --start START [START ...] Starting GPS times(required) --duration DURATION Duration (seconds) [10] -c FRAMECACHE, --framecache FRAMECACHE use .gwf files in cache not NDS2, default use NDS2 --highpass HIGHPASS frequency for high pass butterworth, default no filter --secpfft SECPFFT length of fft in seconds for each calculation --overlap OVERLAP Overlap as fraction [0-1) --nologf make frequency axis linear, default=logarithmic --fmin FMIN min value for frequency axis --fmax FMAX max value for frequency axis --nology make Y-axis linear, default=logarthmic --ymin YMIN fix min value for yaxis defaults to min of data --ymax YMAX max value for y-axis default to max of data -g GEOMETRY, --geometry GEOMETRY size of resulting image WxH, default: 1200x600 --interactive when running from ipython allows experimentation --title TITLE One or more title lines --suptitle SUPTITLE 1st title line (larger than the others) --xlabel XLABEL x axis text --ylabel YLABEL y axis text --out OUT output filename, type=ext (png, pdf, jpg), default=gwpy.png --legend [LEGEND [LEGEND ...]] strings to match data files --nolegend do not display legend --nogrid do not display grid lines .. rubric:: Next .. toctree:: :maxdepth: 1 coherence.rst