1. Manuals
  2. Tumbleweed
  3. lalframe-devel
  4. lalfr-vis(1)

Scroll to navigation

LALFR-VIS(1) LALFrame LALFR-VIS(1)

NAME

lalfr-vis -- visualize frame data

SYNOPSIS

lalfr-vis
--channel=channel --frame-cache=cachefile


          --start-time=tstart --duration=deltat [--output=outfile]


          [--highpass=minfreq] [--lowpass=maxfreq] [--pad=padding]


          [--resample=srate] [--spectrum=resolution]


        
lalfr-vis
--channel=channel --frame-glob=globstring


          --start-time=tstart --duration=deltat [--output=outfile]


          [--highpass=minfreq] [--lowpass=maxfreq] [--pad=padding]


          [--resample=srate] [--spectrum=resolution]

DESCRIPTION

The lalfr-vis utility reads a requested interval [tstart,tstart+deltat) of channel data from frame files that are either indexed in the cachefile or matching the pattern globstring as described by glob(3). The output is written to outfile and the format of the output is determined by extension of outfile as described below. If outfile is not specified, the output is written to the standard output in two-column ascii format data.

The lalfr-vis can optionally perform certain manipulations of the data that is read, including:

High-pass filtering of the data.
Low-pass filtering of the data.
Resampling of the data.
Computing the power spectrum of the data.

If any of the filtering or resampling operations are performed, it is recommended additional padding is used. This additional data, before and after the requested interval, will be discarded before output (or before computing the power spectrum) which will remove filter transients. Note that data will be read for the entire interval [tstart-padding,tstart+deltat+padding) and must be available.

OPTIONS

Prints the help message.
The channel name that is to be read.
The cachefile indexing the frame files to be used.
The cachefile indexing the frame files to be used.
-o outfile, --output=outfile
The outfile to use. The extension of outfile is used to determine the format of the output. The output formats are described below.
The time tstart GPS seconds of the data to read. If padding is specified with the -P option or the --pad option, an additional amount of data preceding tstart is also read, and discarded after any requested filtering of the data is complete.
The duration deltat in seconds of data to read. If padding is specified with the -P option or the --pad option, an additional amount of data is also read, and discarded after any requested filtering of the data is complete.
High-pass filter the data at minfreq Hertz. An additional amount of data, which will be discarded after the filtering, should be specified with the -P option or the --pad option to remove filter transients.
Low-pass filter the data at minfreq Hertz. An additional amount of data, which will be discarded after the filtering, should be specified with the -P option or the --pad option to remove filter transients.
Read padding additional seconds of data before and after the requested interval. This data is then dropped after all requested filtering has been performed in order to remove filter transients.
Resample the data to sampling rate srate Hertz. An additional amount of data, which will be discarded after the filtering, should be specified with the -P option or the --pad option to remove filter transients.
Compute the power spectrum of the data at the requested resolution in Hertz. Depending on the output format, either the amplitude spectral density or the power spectral density is output.

OUTPUT FORMATS

If the -o or --output option is used to specify an output file, the extension of that file is used to determine the output format. Supported output formats include:

.au
Au audio file format. This format is for time-series data only and may not be used if the -S or the --spectrum option is used.
.eps
Encapsulated PostScript (EPS) graphical file format. A plot of the data values as a function of time is produced using the gnuplot(1) program, if available. If the -S or the --spectrum option is used, a log-log plot of the amplitude spectrum is produced instead.
.gif
Graphics Interchange Format (GIF) graphical file format. A plot of the data values as a function of time is produced using the gnuplot(1) program, if available. If the -S or the --spectrum option is used, a log-log plot of the amplitude spectrum is produced instead.
.jpg
JPEG graphical file format. A plot of the data values as a function of time is produced using the gnuplot(1) program, if available. If the -S or the --spectrum option is used, a log-log plot of the amplitude spectrum is produced instead.
.pdf
Portable Document Format (PDF) graphical file format. A plot of the data values as a function of time is produced using the gnuplot(1) program, if available. If the -S or the --spectrum option is used, a log-log plot of the amplitude spectrum is produced instead.
.png
Portable Network Graphics (PNG) graphical file format. A plot of the data values as a function of time is produced using the gnuplot(1) program, if available. If the -S or the --spectrum option is used, a log-log plot of the amplitude spectrum is produced instead.
.ps
PostScript (PS) graphical file format. A plot of the data values as a function of time is produced using the gnuplot(1) program, if available. If the -S or the --spectrum option is used, a log-log plot of the amplitude spectrum is produced instead.
.svg
Scalable Vector Graphics (SVG) graphical file format. A plot of the data values as a function of time is produced using the gnuplot(1) program, if available. If the -S or the --spectrum optione used, a log-log plot of the amplitude spectrum is produced instead.
.wav
Waveform Audio File Format (WAVE) audio file format. This format is for time-series data only and may not be used if the -S or the --spectrum option is used.
.xml
XML-based LIGO-lightweight (LIGOLw) file format. If the -S or the --spectrum option is used, the power spectral density data is written to the file.

If none of these extensions are used then the output will be in two-column ascii format. The first column will be the GPS time of each sample of data and the second column will be the sample values. However, if the -S or the --spectrum option is used, the first column will be the frequency of each sample of the spectrum and the second column will be the value of the power spectral density at that frequency.

ENVIRONMENT

The LAL_DEBUG_LEVEL can used to control the error and warning reporting of lalfr-vis. Common values are: LAL_DEBUG_LEVEL=0 which suppresses error messages, LAL_DEBUG_LEVEL=1 which prints error messages alone, LAL_DEBUG_LEVEL=3 which prints both error messages and warning messages, and LAL_DEBUG_LEVEL=7 which additionally prints informational messages.

EXIT STATUS

The lalfr-vis utility exits 0 on success, and >0 if an error occurs.

EXAMPLES

The command:

lalfr-vis -c H1:LSC-STRAIN -g "H-*.gwf" -s 1000000000 -t 16 -o out.wav

will read 16 seconds beginning at GPS time 1000000000 of H1:LSC-STRAIN data from frame files matching ``H-*.gwf'' in the current directory and ouput the data as a WAVE audio file out.wav.

The command:

lalfr-vis -c L1:LSC-STRAIN -f LLO.cache -s 1000000001 -t 64 -R 2048 -H 10 -L 1000 -P 1 -S 0.25 -o out.png

will read 66 seconds beginning at GPS time 1000000000 of L1:LSC-STRAIN data from frame files indexed in LLO.cache, and the following manipulations will be performed: the data will be resampled to a sampling rate of 2048 Hz, the data will be high-pass filtered at 10 Hz, the data will be low-pass filtered at 1000 Hz, the first and last 1 second of data will be dropped (to remove filter transients), a power spectrum will be computed with 0.25 Hz resolution, and a PNG file displaying a log-log plot of the amplitude spectral density will output in file out.pnd.

SEE ALSO

gnuplot(1), lalfr-stream(1)

AUTHOR

Jolien Creighton

10 June 2013 LALFrame