Output of .was and .wdr Files

by KurtRosenberger last modified Sep 25, 2007 10:51 AM
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Output of .was and .wdr Files

Posted by KurtRosenberger at August 16. 2007
Hi there,
Can someone tell me how the amplitude and direction reported in the .was and .wdr are derived? Is this a simple PUV, or some averaged version of the full directional spectra as calulated by MLM-AST?

Cheers

Kurt
Current state: Being created

Output of .was and .wdr Files

Posted by KurtRosenberger at August 17. 2007
Hi there,

Torstein is back on Monday -- he will probably give the better answer  <img src=" />:)'>

- Atle Lohrmann
Current state: Being created

Output of .was and .wdr Files

Posted by KurtRosenberger at August 20. 2007
Hi Kurt,

I am guessing that you are using QuickWave to process you wave data.  There is a help button in the dialog box which provides you with the information that you requested.  I will recap here since it is useful for anyone using Quickwave.

Energy Density Spectra
The Energy Density Spectra is output in the *.WAS file.  The units are meter^2/Hz.  The ASCII file is intended to be easily read into MatLab or Excel, where the first row contains the frequencies of each estimate and each of the following rows is the energy spectra for each wave burst measurement.

The user can select which measurement the enegy density is based; The options for the AWAC are Acoustic Surface Tracking, Pressure, Velocity, or Optimized.  The optimized setting uses AST as the primary unless one of the quality control checks deems the AST too poor to use, in this case the energy estimate is falls back on either the pressure (depth < 20 m) or velocity measurements (depth > 20 m).

For PUV instruments (Aquadopp Current Meter, Aquadopp Profiler, Vector), the pressure is the only measurment used for energy estimates.

Direction Spectra
The Direction Spectra is output in the *.WDR file.  This file contains an estimate of the mean direction at each frequency.  The units for this is degrees, and reference to magnetic North.

The processing method for the direction is either the SUV or MLM-ST (for AWACs with AST), MLM (non-AST AWACs),  or PUV (Aquadopp Current Meter, Aquadopp Profiler, Vector).

kind regards,
Torstein
Current state: Being created

Output of .was and .wdr Files

Posted by KurtRosenberger at August 23. 2007
Hi Torstein,
Thanks for the reply. I did check the help file, and it does not outline the method used to get the directions in the .wdr file. It lists the output as being "directional spectra", but not full directional spectra (energy by degree and frequency bin). So you're saying the mean direction is also an output of the MLM method?

Thanks

Kurt
Current state: Being created

Output of .was and .wdr Files

Posted by KurtRosenberger at August 24. 2007
Hi Kurt,

I think there are two points of confusion here (1) directional spectra (*.WDR) may be confused with full directional spectra (*.WDS), and (2) it looks like the edits to the help file never "took" the last time I compiled QuickWave  :angry:

I have pasted in the section covering output files below.  The part on the WDS files discusses what the contents are and how to use it to get the energy density per degree-frequency bins.

on a side note, the directional spectra in the *.WDR file is the mean direction at each frequency; these values are based on the first pair of Fourier coefficients (A1 & B1).  The energy distribution found in the *.WDS file is based on the first two pairs of Fourier coefficients (A1, B1, A2, B2).  The directional processing method to arrive at these Fourier coefficients is selected by the user in the processing parameters option of QuickWave.  The processing settings used are also indicated in the Header file (*.WHR).

Sorry for the confusion with the help file.  Below is what you are looking for.

regards,
Torstein

-------------------- QuickWave File Output ----------------


There are several output files available from QuickWave.  The user has the choice of which files will be output.  There is one file which is always output, this is the header file FILENAME.WPR.  The header file contains information on how the instrument was configured, the parameters used for wave processing, and a description of the remaining output files.

Wave parameter file *.wap[/U]
This file presents the estimates of the standard wave parameters for each wave burst measurement a description can be found in the section on Definition of standard wave parameters.

Wave engery spectra file *.was
This file presents the energy spectra for each burst and begins with the frequency values used (Hz).  The units for the energy spectra are (meter2/Hz).  The spectra used for this is described in the section Definition of standard wave parameters.  Note that the frequency limit (Nyquist) for this spectra can be greater than the directional spectra if the measurements include the Acoustic Surface Tracking (AST); this is because the AST samples at twice the frequency as the standard measures of pressure and velocity.

Wave directional spectra file *.wdr
This file presents the direction at each frequency, or the “directional spectra” for each burst and begins with the frequency values used (Hz).  The units for the energy spectra are (degrees).

Wave full directional spectra file *.wds
The full directional spectra file is a presentation of energy distribution over both direction and frequency.  This is sometimes of interest when viewing the distribution as a contour plot.  This file tends to be quite large and therefore is often not output unless used.  The units are normalized and reported as (Normalized-Energy/degree), this means that if the directional spectrum for single given frequency was integrated from 0 to 360 degrees, then the result would be 1.  

In order to calculate the full energy-direction spectrum, one must multiply the results from the energy spectra with the normalized full directional spectra.  This would provide the units of meter2/Hz /degree.  The full directional spectra is reported as normalized spectra because the file size would be enormous if we tried to cover all sea states with the required significant figures (i.e. dynamic range demands here are considerable).

It is possible that the Energy spectra file has a frequency range that this greater than that found in the full directional spectra.  This has to do with the different Nyquist limits for the directional and non-directional spectra when using AST spectra.  Matching frequency lengths can be achieved by setting the upper frequency limit (Processing parameters) below the Nyquist limit for the directional spectra.

Wave Fourier coefficient file *.wcf
This file presents the first two Fourier coefficient pairs at each frequency.  This data is useful if one intends to perform further post processing of directional estimates.

Wave time series file *.wst
This file presents the AST time series after it has been cleaned up with the despiking routines.  This means the bad detects have been identified and linearly interpolated by the neighboring values that are considered acceptable.  This file tends to be large so it is not necessary to output unless intended to be used.
Current state: Being created

Output of .was and .wdr Files

Posted by KurtRosenberger at August 24. 2007
I did see that section in the help file, but it was not detailed enough (i.e., it doesn't explicitly state that the direction in the .wdr file is a mean direction based on the first two Fourier coefficients). Thank you - that was the information I was looking for. I just want to be able to provide the correct metadata when I write the processed data out to netCDF.

Cheers

Kurt <img src=" />:D'>
Current state: Being created

Output of .was and .wdr Files

Posted by KurtRosenberger at August 31. 2007
One other question - does the fourth beam measure along-beam velocity also? I've read papers that show how to get turbulence estimates from different beam configurations, and I was under the impression that Beam 4 on the AWAC also measured velocity (which I understand is a better measurement of vertical velocity?), but I don't see it in the output...

Kurt
Current state: Being created

Output of .was and .wdr Files

Posted by KurtRosenberger at September 25. 2007
Hi Kurt,

We have actually decided to not measure along beam velocity for the vertical beam.  The reason for this is that the three beams at an angle are sufficient for determining the 3D flow during the current profiling mode and more importantly we do not transmit on this transducer and thus save 30% power during current profiling.

As you already know, the reason we have the vertical pointing beam is for the Acoustic Surface Tracking which would not really work that well for the non-vertical beams.  In wave mode the transducer is dedicated for AST and not the velocity.

When comes to turbulence studies, we have found the velocimeter to be a better instrument because of its (a) higher sampling rate, (b) smaller measurement volume, © measurements are not spatially separated as with a current profiler.

hope this helps,
Torstein
Current state: Being created
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