Acoustics Toolbox

In addition, AT contains BOUNCE, which computes the reflection coefficient for a layered medium and may be used to provide input to BELLHOP. A common input structure has been used throughout so that only minor modifications are needed to switch from one program to another.

All the models produce `shade' files that can be processed using a common set of plotting routines to plot transmission loss vs. range or vs. range and depth.

Porting the code

Depending on your platform, you may be able to execute the pre-compiled binaries. Currently we use GFORTRAN to compile those. However, our version requires access to gcc dynamic libraries. Therefore, you will need to have a compatible version of gcc and gfortran installed on your system to run the pre-compiled binaries.

The package adheres quite strictly to the latest Fortran standard. If you use an older Fortran such as Fortran 77 you will have problems. You will also likely encounter a few issues if you go back to Fortran 90.

Record length

Fortran compilers differ in whether record lengths should be declared as bytes or words. To ensure the programs run, I declare lengths in bytes. If your compiler uses words as the default, look for a compiler switch to override that so that your files are not unnecessarily large.

Some of the programs in this package use direct access I/O and need to know a record length. Many systems do not maintain this information as part of the file info so the code writes that information directly into the file. Then the file is opened twice. First it is opened with a dummy record length to read the actual record length from the file. Then it is re-opened with the correct record length. On machines that do know the correct record length, that first open may generate an error message and will have to be removed. The RECL specifier should then also be removed from the second open.

Plotting:

Plot packages come and go. However, the output formats of the various models are all fairly simple to work with. The distribution includes Matlab scripts which I currently use for plotting. If you don’t have Matlab, then these will at least provide an example of how to read the file formats.

Installation Notes

To run the Acoustics Toolbox, the executables need to be in your path. The process for setting your path depends on your operating system. I can't stay current with the options but here are some things that have worked in the past:

DOS: add the following to your autoexec.bat to make the scripts executables in your default path:

Windows 2000 (and perhaps NT): right click on the “My Computer” icon and select “Properties”, “advanced”.

Windows XP: go to control panel/Performance and Maintenance/System/Advanced and look for the pushbutton labled “Environment Variables”. There you can edit the system variable “Path”.

Obviously these lines should be updated to reflect whichever directory you installed things in. You may need to reboot to make sure this takes effect. Note that the DOS and Unix scripts are not maintained. We currently execute the binaries via Matlab.

If you’re having problems, verify your path includes these by typing “path” from a DOS window. Typically you run KRAKEN by typing something like “kraken pekeris”. at the DOS command line, or kraken( 'pekeris') at the Matlab command line.

Finally, if you use Matlab then you just need to use the "Set Path" option under the "File" menu. If you include all of the Acoustics Toolbox in your Matlab path, then the Matlab scripts find the location of the binaries using the Matlab "which" command.

Once you have the basic code working, you might want to run some of the test batteries in at/tests to completely verify your installation. The m-file, runtests.m runs the complete suite of tests using the Fortran binaries. The m-file runtestsM.m does the same thing, using the Matlab versions of BELLHOP, SCOOTER, BOUNCE, and SPARC.

Updates

(Check also the individual sub-directories for updates on individual components of the Acoustics Toolbox.)

Minor changes have been made to the package for improved f77 to f90 portability. Fortran 90 seems to treat parameters differently in terms of precision so some of those changes are important for the most accurate results.

The whole package has been converted to f90/95 standard with free-format lines and taking advantage of dynamic allocation. The code is more concise and portable. Dynamic allocation means that you will not have to worry about dimensional limits--- the size of the problem you can solve is limited only by RAM on your system.

The change to dynamic allocation has forced a small change in the input structure. Previously an input format was often used with a number of items in a vector followed by the actual vector. For instance, the vector of receiver depths is read this way.

In the new version the number of items in the vector must appear on a separate line so that the code can read it, allocate the space, and then read the vector contents.

The Matlab version of BELLHOP has been replaced by a new version that traces one beam at a time. The earlier version traced all the beams in parallel for efficiency; however, the logic is too complicated to maintain.

Converted most "char foo*5' references, which are deprecated in the new Fortran, in favor of "char (len=5) :: foo".

Updated the volume attenuation from the 1967 Thorp formula to the more recent one in JKPS. Converted all the Fortran models so that they would determine the file names from the command line arguments. This eliminates the need for DOS, Unix, or Matlab scripts to move files around.

Made all type conversions, e.g. complex to real or double to single, explicit. Expanded use of EXPLICIT NONE to ensure all variable types are called out. Further expansion of the lengths of variable names to take advantage of Fortran 2003. Expanded use of structure-variables. Additional changes as described in the read.me files for the various models. This is a fairly significant revision in terms of the evolution from Fortran 77 to Fortran 2003. However, there are virtually no changes to the input and output files.

Greatly expanded use of INTENT( IN, OUT, etc.) to clarify the source code. Continued changes in variable and subroutine names to make them more readable as the Fortran 2003 standard permits. Use of explicit dimension sizes in variable declarations to make it easier for the compiler to detect incompatibilities. Change to SHDFile format for the pressure field to allow multiple x-y coordinates for the source.

Added an option for a source beam pattern in KRAKEN and SCOOTER. The pattern is read from a file, following the same procedure as in BELLHOP. The beam pattern is actually introduced after the KRAKEN or SCOOTER run by processing the mode file (FIELD and FIELD3D) or the Green's function file (FIELDS). Currently the beam pattern is implemented by shading the wavenumber spectrum. As a result the beam pattern must be symmetric with respect to the horizontal (only the part of the pattern with positive angles is used). This capability has also been implemented in the Matlab versions of FIELD and FIELDS; however, in FIELD it current only works for the range-independent case.

The new Matlab changed how it did shell escapes (to run things at the command line level) so that piping of stdin and stdout no longer worked. To get around this FIELD and FIELDS have been modified so that they read from a user specified file instead. The field parameter information is now read from 'root.flp' instead of field.flp, where 'root' is the root of a filename passed to the code. This change has been made in both the Fortran and Matlab versions. In addition, to make the Matlab more compatible with the Fortran version, the various output files (SHDFIL.mat, GRNFIL.mat, etc.) now use individually named files (root.shd.mat and root.grn.mat, etc.).

February 2013
A bug was fixed in detecting the end of the SSP for a given layer. Instead of testing for exact equality of the SSP depth to the bottom-depth of the layer, I had previously checked for agreement to within a tolerance. The tolerance was scaled based on the bottom depth of the layer so for a bottom depth of zero (in an aero-acoustic problem) the tolerance was 0 and the bottom was not detected.

February 2014
Checks have been added to ensure certain vectors are monotonically increasing where that assumption is critical to the codes.

November 2014
The Matlab routines that read altimetry and bathymetry files were not clearing old data on subsequent calls. This occurred only when the flat boundary was selected and the routines were supposed to return dummy boundary information. Also, the ranges were not being converted to meters from kilometers. It effected SimplePE runs and probably the Matlab version of BELLHOP as well. These routines are not used by any of the Fortran implementations and the error often had no effect on the Matlab codes.

June 2014
Sometime around January of 2010 the Thorp formula for volume attenuation was modified at the request of a user. The modified formula was slightly more accurate. The change was verified in BELLHOP; however, there an incorrect variable name was used in the crci routine used by KRAKEN and SCOOTER. That error mean the added Thorp attenuation was never added. This is corrected in the new code. The volume attenuation was typically most important for higher frequency sources, which in turn were more often treated in BELLHOP. However, the error can be important for low frequency sources at very long range.

July 2017
The package has been modified to allow broadband runs for most of the models. Thus, for example, you can give a vector of frequencies to KRAKEN or SCOOTER and produce a single pressure file containing results for each of the frequencies. This has required a small change to the file formats for modfils, shdfils, grndfils, etc. In addition, all the Matlab codes have been modified to allow the '/' convention used in the Fortran versions. This option allows a user to either specify a full vector or just specify the upper and lower limits terminated by '/'. It then uses those limits to create a vector of equally spaced points.

November 2017
Updates and fixes to the noise routines in at/Matlab/noise. A routine has been added to construct the noise covariance matrix directly from the shdfil. The shdfil contains the complex pressure field vs. range and depth and the noise routine can use such files produced by KRAKEN, KRAKENC, SCOOTER, and BELLHOP.

March 2018
SimplePE was not updating the marching matrices in the case where there was a range-dependent SSP but a flat bottom. Fixed ...

November 2018
A Piecewise-Cubic Hermite Interpolating Polynomial (PCHIP) option has been added for interpolating the SSP in the various models. This is really motivated by BELLHOP. The beam tracing algorithm can be sensitive to the profile interpolation. Ideally the interpolation should produce a smooth profile and the c-linear and n2-linear options are only piecewise linear so they have discontinuities in their first derivatives. The spline option is smooth (up to second derivatives) but in some cases produces contorted interpolants to achieve that smoothness. The PCHIP option sacrifices some smoothness for better behavior. This has been implemented in all the Fortran codes. The Matlab versions are not current. i.e. do not have this implemented; however, it is an easy modification.

There are many varieties of PCHIP; the earlier spline option is one of them. A popular PCHIP is based on work by Fritsch and Carlson and produces a monotonic curve between data points--- so does not introduce new extrema. The key in that implementation is to replace nodal derivatives with zero if there is a sign change in the derivative between adjacent segments. There are also variations in how the endpoints are treated. The monotonic pchip did not have the effect I wanted. I've gone with a simpler piece-wise cubic that simply averages the derivatives between adjacent segments. That average is not O(h^2) if the grid is varying. However, there are physical arguments that motivate the simpler average and I didn't see a benefit in spending more time on that.

January 2019
For those of you working at a lower level with the software, note that vectors that previous referred to source and receiver depths now refer to a z coordinate, e.g. Pos.r.depth becomes Pos.r.z. This change was motivated by BELLHOP3D, which uses x, y, and z coordinates for sources and receivers--- it made the code structure more consistent in the sense that (x,y,z) makes more sense than (x,y,depth). This change is transparent to you unless you're using some of the Matlab scripts to read the shade files into your own Matlab code.

John Peterson worked further on the PCHIP implementation and made an implementation faithful to the original PCHIP and consistent with the Matlab version. He also implement PCHIP in the Matlab versions of SCOOTER, SPARC, and BELLHOP.

February 2019
Volume attenuation in the ocean had been implemented using the Thorp formulas. A new option has been added to use to more refined formulas due to Francois and Garrison (1982). This has been implemented in all the Fortran models (Kraken, Scooter, Sparc, Bellhop, Bounce) as well as their Matlab equivalents. I have only checked the Bellhop and Scooter implementations.

May 2019
The 'm' option for attenuation (in dB/m with a transition to a power law at a transition frequency) was no longer working. I was testing the AttenUnit (two-letters) option for equality to the single letter 'm', so it was never being invoked. This error was in ReadEnvironmentMod and obviously crept in after the original implementation.

The Francois-Garrison volume attenuation had been implemented in the Matlab codes using hard-wired values for Temperature, Salinity, pH, and depth. The codes have been modified to read those values from the envfil in a manner consistent with the Fortran codes.

This should be transparent to the user, but a common routine was written for the Fortran to read a vector (ranges, bearings, ray angles, etc.). This routine echoes the data to the print file, skipping intermediate points if there are many elements. It also converts values for ranges in km to m since the package uses meters for internal units. It allocates dynamic variables and generates intermediate values by linear interpolation if the user has used the '/' option where only the first and last values of the vector are provided. That code had been repeated in a lot of places so this simplified and unified the code a great deal, but involved a lot of changes.

The matlab version of 'field' and the associated 'evalri' that implemented the modal sum has been cleaned up. It runs a lot faster now and allows multiple source depths and broadband (multi-frequency) cases. Note that the documentation pertains still to the Fortran version of field and that not all of the capabilities are implemented in the Matlab version.

A 'call flush' statement has been added to the main codes so that print statements that show the progress of a run are flushed to the print file. Without that, the output is buffered and you can't monitor the progress.

July 2019
The shdfil created by the various models is a direct access file and was being opened with STATUS='UNKNOWN'. As a result, if the file already existed it was used without change. This meant it kept its original size even if it no longer needed the same storage space. This problem was fixed by opening the files with STATUS='REPLACE'. A similar problem had happened previously with the KRAKEN modefiles and had been fixed in KRAKENC, but not KRAKEN.

This version has a significantly better version of the PCHIP (Piece-wise Cubic Hermite Interpolating Polynomial) for interpolating the SSP and related info. I had done a preliminary implementation but it was not faithful to the true PCHIP. Also the newer PCHIP is more sophisticated, producing a blend of the cubic spline and the traditional PCHIP that seems to offer the best of both. (Thanks to J. Peterson.) This change is relevant to all the models, but particularly significant for BELLHOP since ray-based models tend to be more sensitive to the SSP interpolation.

December 2019
In preparing an update, I found an access in SPARC outside of the declared length of the source-depth vector. This problem was due to the fact that the time-domain code SPARC tried to treat the times for snapshots as source depths. To be more consistent, the entire package now treats frequency as a conjugate variable to time, and range as a conjugate variable to the horizontal wavenumber. This unifies the file formats for grnfil, shdfil produced by SPARC, SCOOTER, KRAKEN, etc. Wherever frequency occurs, SPARC uses that space for time; wherever range occurs, SCOOTER and SPARC use that space for the horizontal wavenumber. Routines such as fieldsco.m Fourier transform those output fields to the conjugate variables, preserving the basic file structure.

There had been some fussy code in broadband runs where the first element of a frequency vector was used to denote a carrier frequency. The broadband codes now use a separate variable, freq0, for the carrier or nominal frequency to avoid confusion. That scalar frequency is also now separately written to the output shdfil or grrnfil.

June 2020
A user inadvertently selected a very large attenuation in a sediment layer. That attenuation is combined with the real sound speed to generate a complex sound speed, taking into account the user units. If the resulting complex sound speed has an imaginary part greater than the real part, then the squared sound speed is in the negative halfplane. This is not physical and creates errors. A trap has been added to detect and flag this sort of error.

October/November 2020
There was a mismatch in the number of arguments for a call to ANALYT in at/misc/sspMod.f90. This option for an analytic SSP was rarely used; however, the mismatch caused a compiler error under gfortran10. I fixed one such call in October; however, in November the error persisted and was tracked to a second call. (I had been using gfortran 9.0 and did not encounter the problem.)

June 2021
A couple of years ago I changed the Position variables (Pos.s, Pos.r for source and receiver) to use (x, y, z), rather than (x, y, sd) and (x, y, rd). So Pos.s.rd is now Pos.s.z for example. This is just a more self-consistent notation. This change affected many, many Matlab scripts. I changed the ones I was using; however, there are lots of other ones that are rarely used, but which people sometimes stumble upon. Laurel did a global replace so that there should no longer be any remnants of the old variable names anywhere in the code.

April 2022
After upgrading the MacOS to Monterey we are finding that the model executables produced by gfortran are no longer consistently flushing the buffers for output files. The Fortran standard seems to indicate this should happen automatically but it is not clear if this is a problem in gfortran or the new MacOS. I have added FLUSH and CLOSE statements in appropriate places in the code and this seems to have resolved the problem. This problem did not occur with the Intel compiler.

August 2022
As mentioned above gfortran has not been consistently flushing buffers. The main programs have 'close' statements at the end to deal with that. However, in cases of fatal errors the termination is handled by a separate routine that was missing a close statement. So in such cases the output file was empty providing the user with no information about why the program stopped. A 'close' statement has been added there as well. This problem did not occur with the Intel compiler

October 2022
A user ran into a problem simulating a horizontal array at near-broadside because the receiver ranges were nearly identical to within millimeters. In fact, when the receiver offsets were added to the nominal range of the array, the hydrophones appeared to all be at identical ranges because the ranges are stored in single precision internally. There is a test when this input is read to see if the ranges are strictly monotonically increasing and then -- depending on the particular model -- the code would abort with a fatal error.

It's not clear if strict monotonicity is required, but, for instance, some of the BELLHOP beam options implicitly assume the ranges do not decrease anywhere. In addition, some of the plotting routines will likely be confused if the ranges are not increasing. For now, the monotonicity test is being left in; however, the range vector has been converted to double precision. That higher precision is rarely going to matter, but it does mitigate this particular problem. At some later point, I may change all the Position vectors to double precision to be conservative. However, in some cases this would unnecessarily double the file size and that is often a concern for our global acoustic modeling.

A little more clean-up on the double precision source/receiver positions mentioned just above ... Anything related to the x-y coordinate of a source or receiver is now double precision. This includes the source lat./long. and receiver bearings. The SCOOTER Green's function file (GRNFIL) likewise has wavenumbers in double precision as the wavenumber vector is sort of the dual of the range vector. These changes may improve the accuracy for high-frequency cases and when sources are not at the origin. (When sources are not at the origin a set of bearings may result in small range offsets added to a large origin coordinate.BELLHOP3D and KRAKEN3D/FIELD3D allow sources to be at arbitrary locations.) Some other variables (frequency and attenuation) were also converted to double precision.

In unusual cases, this change may result in larger output shade files. This would happen, for instance, if the field were computed on a very large number of bearings so that the vector of bearings rather than the vector of ranges determined the record size.

Source and receiver depths have been left in single precision for now; I thought the precision was much less likely to be an issue there and there were some worries about side-effects in changing that.

Frequently Asked Questions

You left off a carriage return/line feed after the last line, or other appropriate end-of-line marker for your system. There are other ways this could happen; check the print file to see where you deviated from the expected format. The models try to echo the input as soon as its read, so you can see clearly where the error happened.

Generally you should never see this. However, if you ran a case that required an outrageous amount of storage you might encounter a problem. The code is supposed to catch all such cases by detecting an error in the allocation of dynamic variables (or limits for the few arrays with fixed dimensions). However, we see cases where the compiler simply does not handle huge arrays properly.

The source is s( t ) = e(+i \omega t ) in the Acoustics Toolbox models. This is the opposite convention of what we used in the book Computational Ocean Acoustics. We had to standardize on one convention and the models we used were inconsistent.

The KRAKEN manual mimics the book in terms of the theoretical presentation— the footnote on p. 6 of the manual is to warn the user that the code has the opposite sign convention.