Difference between revisions of "Utilities"
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= HDFview =  = HDFview =  
−  * HDFview is a free  +  * HDFview is a free visualization tool for browsing and editing HDF4 and HDF5 files. 
* To download or download a free copy visit:  * To download or download a free copy visit:  
−  :  +  : https://www.hdfgroup.org/downloads/hdfview/ 
+  
+  *Later HDFView binaries require C++ redistributables. If you install the viewer and still cannot access the files, try installing this:  
+  : https://support.microsoft.com/enus/help/2977003/thelatestsupportedvisualcdownloads  
= Grain Size Distribution Analysis =  = Grain Size Distribution Analysis = 
Latest revision as of 17:16, 5 March 2020
Time Series Analysis
Filter1D: Time Series Analysis Tool
 The Matlab utility provides users of the SMS, a onestop package for preparing model input time series and allows users to interpolate, resample, filter, and transform any type of model forcing and supports SMS compatible file formats for ease of data transfer.
 The main feature of the software is the ability to apply highpass, lowpass, bandpass, and bandstop filters to time series.
 Filter1D uses a windowed sinc filter which is a nonrecursive finite impulse response filter.
 Wiki Manual Filter1d
 PDF User Guide filter1d_userguide.pdf
 Download Matlab script filter1d.m
 Download Matlab executable filter1d.exe
 Link to download Matlab Compiler Runtime library: http://www.mathworks.com/products/compiler/mcr/
 Download sample time series data file Blind_Pass.tsd
TAP: Tidal Analysis and Prediction software
 TAPtides is the ideal package to explore and develop preliminary or finalized tidal predictions from serial records spanning several weeks to several months.
 Designed to be easy to use, its Graphical User Interface permits quick separation of a time series of water level measurements into its tidal and nontidal components using a selective least squares harmonic reduction employing up to 35 tidal constituents.
 After saving the tidal constants for the constituents selected during analysis, the user can generate predictions of the astronomical tide, the water level that varies at known tidal frequencies attributable to gravitational interactions between the earth, moon, and sun.
 Wiki Manual for TAPtides TAPtides
 Wiki Manual for TAPcurrents TAPcurrents
 Download software TAP.rar
Matlab scripts
Read CMSFlow Grid File (*_grid.h5)
 cms_read_grid.m Reads a CMS nonuniform Cartesian grid
 Description:
 Reads a CMS grid file and creates a structure variable containing the grid variables
 Usage:
 grd = cms_read_grid(filename);
 Input:
 filename  Input file name including full path (e.g. 'Flow_grd.h5')
 Output:
 grd  structure variable containing the following variables
 nx  Grid size in x direction []
 ny  Grid size in y direction []
 x0  Grid origin in x direction [m]
 y0  Grid origin in y direction [m]
 angle  Grid angle [deg]
 x(1:nx)  Cellcenter coordinates in x direction [m]
 y(1:ny)  Cellcenter coordinates in y direction [m]
 depth(1:ny,1:nx)  Cellcentered depth [m]
 active(1:ny,1:nx)  Cell activity (1active and 0inactive) [logical]
 Plus other optional datasets such as mannings, d50, etc.
 Author: Alex Sanchez, USACEERDCCHL
 Download Matlab script cms_read_grid.m
Read CMSFlow Tel File (*.tel)
 Description:
 Reads a CMS telescoping grid file and output all variables to a structure array.
 Usage:
 out = cms_read_tel(telfile);
 Input:
 telfile  Telescoping grid file including path (*.tel)
 Output:
 tel  Structure including the following fields
 ncells  Number of cells
 x0  Grid origin in xdirection [m]
 y0  Grid origin in ydirection [m]
 angle  Grid angle [deg]
 id  Cell ID number
 x  Grid cellcentered coordinate in xdirection [m]
 y  Grid cellcentered coordinate in ydirection [m]
 dx  Grid cell resolution in xdirection [m]
 dy  Grid cell resolution in ydirection [m]
 iloc  Cell connectivity
 depth  Cellcentered depths (999 = inactive cell) [m]
 Author: Alex Sanchez, USACE
 Download Matlab script cms_read_tel.m
Read CMSFlow solution files
 Description:
 Reads a CMS solution file and creates a structure variable containing the solution datasets values and times
 Input:
 filename  input file name including full path
 grd  Grid structure containing the following fields
 nx  Grid size in x direction
 ny  Grid size in y direction
 varargin  dataset names
 Output:
 sol  structure variable containing dataset values and times
 varargout  variable length datasets corresponding to varargin
 Usage:
 filename = 'test_sol.h5';
 sol = cms_read_sol(filename,grd);
 wse = cms_read_sol(filename,grd,'Water_Elevation');
 [wse,uv] = cms_read_sol(filename,'Water_Elevation','Current_Velocity');
 sol = cms_read_sol(filename,'grid',grd,'datasetnames',dnames,...
 'points',pts,'cells',ids,'polygon',poly,'steps',nstep,'times',t)
 Author: Alex Sanchez, USACEERDCCHL
 Download Matlab script cms_read_sol.m
 Download sample solution file test_sol.h5
Read SMS Time Series Data File
 Description: Reads the Surfacewater Modeling System timeseries data (*.tsd) file.
 Usage:
 [t,dat,name,units] = sms_read_tsd('data.tsd');
 Download Matlab script sms_read_tsd.m.
Read a CMS Save Point File
 Description:
 Reads a CMS Save Point file
 Usage:
 sp = cms_read_sp(filename);
 Input:
 filename  CMS Save Point file name
 Output:
 sp  Structure with the following fields
 variable  Name of output variable
 reference_time_str  Reference time string in the following format 'yyyymmdd HH:MM:SS'
 reference_time  Reference time
 label  Save point label
 creation_date  Creation date
 horizontal_projection  Horizontal projection
 vertical_datum  Vertical datum
 time_units  Time units
 output_units  Units of output variable
 cms_version  CMS version number
 number_points  Number of points in time series
 names  Names of output points
 xy  Coordinates of output points
 time  Output times
 scalar  Output scalar
 vector  Output vector
 Author: Alex Sanchez, USACECHL
 Download Matlab script cms_read_sp.m.
Write SMS Time Series Data File
 Description: Writes a Surfacewater Modeling System timeseries data (*.tsd) file.
 Usage:
 sms_write_tsd(filenamet,dat,curvename,curvetype);
 Download Matlab script sms_write_tsd.m.
Read SMS XY Series File
 Description: Reads the Surfacewater Modeling System xy series (*.xys) file.
 Usage:
 [x,y,name] = sms_read_xys('data.xys');
 Download Matlab script sms_read_xys.m.
Write SMS XY Series File
 Description: Writes a Surfacewater Modeling System xy series (*.xys) file.
 Usage:
 sms_write_xys(file,x,y,name)
 Download Matlab script sms_write_xys.m.
Bin scatter data
 Description: Averages the x, y, and z values of points within the same bin. The grid used to define the bins may be user specified are calculated based on the extent of the scatter points. The routine is useful for thinning/smoothing large scatter sets such as multibeam or LIDAR data. The binning method is less accurate then the search radius method, but is much faster.
 Usage:
 [x,y,z] = xyzbin(...);
 [x,y,z] = xyzbin('infile',infile,'outfile',outfile,'dx',dx);
 [x,y,z] = xyzbin('x',xin,'y',yin,'z',zin,'dx',dx);
 [x,y,z] = xyzbin('x',xin,'y',yin,'z',zin,'dx',dx,'dy',dy);
 [x,y,z] = xyzbin('infile',infile,'dx',dx,'x0',x0,'y0',y0,'theta',theta);
 Download Matlab script xyzbin.m.
Interpolation of CMSWave Spectra
 Description: Interpolates the energy spectra in the CMSWave *.eng file to a specified output interval which may be specified in intervals or time units (hours). For example, an output interval of 0.5 index units, interpolates the spectra at half intervals. This subroutine is useful for filling small gaps in CMS spectra.
 Usage:
 interp_eng('Wave.eng','New.eng',1,0.5) %interpolates to every half interval
 interp_eng('Wave.eng','New.eng',1,2) %resamples every two spectra
 interp_eng('Wave.eng','New.eng',2,1) %hrs
 Input:
 engin = Input eng file
 engout = Output eng file
 mode = 1  Index, 2  Time
 dtout = Output steering interval in hours for mode=2 or index for mode 1 (can be less than 1)
 Download Matlab script interp_eng.m.
Principle Component Analysis
 Description: Calculates the principle axes of vector time series data. This subroutine is useful for determining the main direction of fluid flow and extracting the velocity component along the major axis. The principle axes are determined by solving the eigenvalue problem for twodimensional scatter data.
 Usage:
 s = pca2d(u,v)
 Output:
 s = Structure with the following fields:
 center = Ellipse center (centroid)
 area = Ellipse area
 axes = Ellipse axes
 eigen_values = Eigen values
 eigen_vectors = Eigen vectors
 total_variance = Total variance
 percentage_variance = Percentage variance for each axes
 angles = Angles for each axes in degrees
 eccentricity = Ellipse eccentricity
 slope = Slope of the linear fit which goes through the origin
 Note: An alternative simple way of determining the principle axes of vector time series is

(1) 
where and .
 Download Matlab script pca2d.m:.
Data Density Scatter Plot
 Description: datadensity Computes and plots the data density (points/area) of scattered points
 Usage:
 dd = datadensity(x,y,method,radius)
 Input:
 (x,y)  coordinates of points
 method  either 'squares','circles', or 'voronoi'
 default = 'voronoi'
 radius  Equal to the circle radius or half the square width
 Download Matlab script datadensity.m:.
Spectral Analysis
 Description: Calculates the spectrum for a scalar time series using Welch's method. The confidence intervals are calculated with the inverse of chisquare distribution. Also includes a filtering option using the butterworth filter to see the effect of the filter on the spectrum.
 Usage:
 q = specwelch(x,dt,w,Nsg,pnv,Wn,ftype,n);
 [psdf,f] = specwelch(x,dt,w,Nsg,pnv,Wn,ftype,n);
 [psdf,conf,f] = specwelch(x,dt,w,Nsg,pnv,Wn,ftype,n);
 Input:
 x  Time series, [vector]
 dt  Sampling Rate, [scalar]
 win  Window, one of: 'hanning', 'hamming', 'boxcar'
 Nsg  Number of Segments (>=1)
 pnv  Percentage Noverlap of Segments (0100)
 Nb  Band Averaging, number of bands to average
 P  Probability for confidence intervals, (e.g. 0.95)
 Wn  CutOff frequencies, used for filtering
 ftype  Type of filter, 'high', 'low' or 'stop'
 n  Number of coefficients to use in the Butterworth filter
 Output:
 q  structure with the following fields:
 xp  detrended x
 f  Frequencies
 T  Periods
 m  Magnitude
 a  Amplitude
 s  Power spectrum, Sxx(win), [Power]
 psdw  Power Spectrum Density, Pxx(win), [Power/rad/sample]
 psdf  Power Spectrum Density, Pxx(f), [Power/samplefreq]
 psdT  Power Spectrum Density, Pxx(T), [Power*timeunit]
 conf  Upper and Lower Confidence Interval multiplication factors using chisquared approach
 Download Matlab script specwelch.m.
Vector Plot
 Description: Plots directionally correct vectors. Both of matlab subroutines feather.m and quiver.m do not preserve the correct vctor angles.
 Usage:
 h = vecplot(x,y,u,v,'PropertyName',PropertyValue,...)
 h = vecplot(u,v,'PropertyName',PropertyValue,...)
 Input:
 x,y = Position Coordinates
 u,v = Vector Componentes
 Optional Properties
 'DataAspectRatio' = Scaling factor between x and y axes. This is set as the second element of the property 'DataAspectRatio'
 'LengthScale' = Length scaling factor for the barbs or arrows
 'LineSpec' = Line specification string syntax (default 'k^') (e.g. '^k'  plots black arrows, 'k'  plots black sticks)
 'Linewidth' = Linewidth
 'Marker' = '^' for triangle arrows, 'v' for angled arrows,
 and for stick plots (default stick)
 'MarkerFaceColor' = Arrow fill color (default none)
 'MarkerEdgeColor' = Arrow edge color (default line color)
 'MarkerSize' = Marker size
 'LegendLength' = Sets the length of the legend vector
 'LegendUnits' = Sets the units for the legend vector
 'legendPosition' = Sets the legend position (normalized units 01)
 Output:
 h = handles for plot objects
 Download Matlab script vecplot.m.
Tidal Harmonic Analysis
 Description: Simple program which performs a tidal harmonic anlaysis of scalar (e.g. water level) or vector (current velocity) time series. The script is only applicable for relatively short time series of a few months.
 Usage:
 out = tha(in);
 Input:
 in  Structure array with the following fields
 x  real or complex vector [arbitrary units]
 t  time in hrs from zero [hours startin from zero]
 start_time  starting time as [yyyy,mm,dd,HH,MM,SS]
 constituents  optional input constituent names
 rayleigh  optional rayleigh criteria (<=1)
 secular  optional secular correction. Either 'linear' or 'none'. If set to 'linear', the slope is included as a correction to the time series.
 Output:
 out  Structure array with different fields depending on whether the input time series in real or complex.
 amplitudes  Tidal constituent amplitudes (real time series)
 constituents  Tidal constituent names
 equilibrium_arguments  Equilibrium arguments (v+u) for each constituent and starting time
 frequencies  Tidal constituent frequencies
 frequency_units  'cycles/hour'
 nodal_factors  Nodal factors for each constituent and year.
 phases  Tidal constituent phases
 phase_units = 'degrees'
 percent_variance_explained  Percent variance explained of the measured time series by the fitted time series.
 residuals  difference between measured and fit time series
 slope  fitted slope(s)
 speeds  Tidal constituent speeds in degrees/hour
 speed_units = 'degrees/hour'
 time  Julien time in hours from start of year
 time_units = 'hours'
 (variables bewlow are only for complex time series only)
 major_amplitude  Semimajor axis amplitude
 minor_amplitude  Semiminor axis amplitude
 positive_amplitude  Positive axis amplitude (a+)
 negative_amplitude  Negative axis amplitude (a)
 positive_phase  Positive axis phase (phase+) [deg]
 negitive_phase  Negative axis phase (phase) [deg]
 ellipse_inclination  Ellipse orientation or inclination [deg]
 eccentricity
 Version: 3.0
 Date: November 5, 2012
 Author: Alex Sanchez, USACECHL
 Download Matlab function tha.m.
 Download Matlab test script tha_test.m.
 Download tidal data file with nodal factors and equilibrium arguments tide_data_v1.mat.
 Download sample time series file for Crescent City, CA TimeSeries_9419750.txt.
 Download sample constituent file for Crescent City, CA Constituents_9419750.txt.
Extract Time Series from NOAA World Blended Sea Winds
 Description: Extracts a time series of wind speed and direction for use in CMS from the 6 hrly global blended sea wind database (http://www.ncdc.noaa.gov/oa/rsad/airsea/seawinds.html) which has a 0.25º resolution. Outputs *.xys files which can easily be imported into SMS.
 Download Matlab script blended_winds_extract_time_series.m
Image Digitization Tool
 Description: digitize is a user interfase that allows to import image files (.bmp, etc) into MatLab to digitize data from. Previous sessions can also be loaded. It is useful for digitizing plots%and making world files for images. The utility can be used for digitizing time series plots, geographic features such as coastlines, or elevation contours.
 Instructions:
 Load image
 To start a new session, click on the "Load" menu and select "Image File".
 To load a saved session, click on the "Load" menu and select "Session".
 Reference the image
 Click on the "Transformation" menu and select "Add Points".
 Leftclick on the points reference points and Rightclick when finished.
 Rightclick on any reference point and select "Reference" to enter the points "true" coordinate.
 When the coordinated for all the reference points have been entered the "Reference Data Complete" item under the "Transformation" menu will be checked.
 To delete Transformation points, rightclick on a point and select "Delete".
 Digitize Points
 Click on the "Digitization" menu and select "Add Points". The digitized points may be entered at any time, but their transformed coordinated are not calculated until the reference data is complete.
 To see a digitized point's transformed coordinate, rightclick on a point and select "Coordinates".
 Export the Digitized Points
 Click on "Export" and select one of the output options including variables to the workspace and an ASCII file.
 Download Matlab script digitize.m.
Create Spectra Generation Import file with WIS datafiles
 Description: This function creates the .txt file used in the spectra generator of CMS Wave. It prompts the user to select all the desired WIS output files, specify the depth of the station, and whether or not to average the data series. The data and user inputs are manipulated into the format used by CMS Wave file import for spectra generation. Currently the output file is saved in the active directory of matlab.
 Usage: Type mfile name in Matlab command window
 CMS_WIS_to_txt_for_spectragen
 Download Matlab script CMS_WIS_to_txt_for_spectragen.m.
Read an SMS Super ASCII data file (*.dat)
 Description: This function reads an SMS Super ASCII data file (*.dat). These files are part of the SMS Super ASCII format and is an output option for global solution datasets in CMS. The SMS Super ASCII format also includes a coordinates file (*.xy) and a super file (*.sup) which contains the names of the coordinate file and dataset files.
 Usage:
 [t,x] = readsuperdat(filename);
 Download Matlab script readsuperdat.m.
Read an SMS xy file (*.xy)
 Description: This function reads an SMS xy file (*.xy). These files are used in the SMS Super ASCII in conjuction with the by CMS as an ASCII output option for global solution datasets. The SMS Super ASCII format also includes dataset files (*.dat) and a super file (*.sup) which contains the names of the coordinate file and dataset files.
 Usage:
 [t,x] = read_xy(filename);
 Download Matlab script read_xy.m.
Wave Number Calculation
 Description: Simple program which solves the wave dispersion relation sig^2 = g*k*tanh(k*h).
 Usage:
 wk = wavenumber(g,wa,wd,h,u,v,tol)
 [wk,err] = wavenumber(g,wa,wd,h,u,v)
 Download Matlab script wavenumber.m.
TextPad Syntax File for CMSFlow Card File
 Color codes the CMSFlow card file (*.cmcards) so that it is easier to read and avoids misspelling of keywords.
 To setup the file:
 Open Textpad and click on the menu Configure and go to Preferences.
 Click on folder on the left hand side and note the path to the syntax files.
 Copypaste the .syn to the path noted in step 2.
 Click on Configure  New Class Document.
 Enter CMSFlow as the document name and click next.
 Enter *.cmcards in Class members and click next.
 Enable the syntax highlighting and select the CMSFlow_V4.syn file.
 Click on Finish and your done!
 Version 4.0 and earlier: CMSFlow_V4.syn.
 Version 4.1 and earlier: CMSFlow_V4p1.syn.
Notepad++ Syntax File for CMSFlow Card File
 Color codes the CMSFlow card file (*.cmcards) so that it is easier to read and avoids misspelling of keywords.
 Version 4.1 and earlier: CMSFlow_v4p1.xml.
UltraEdit Syntax File for CMSFlow Card File
 Color codes the CMSFlow card file (*.cmcards) so that it is easier to read and avoids misspelling of keywords.
 Version 4.1 and earlier: CMSFlow_v4p1.uew.
HDFview
 HDFview is a free visualization tool for browsing and editing HDF4 and HDF5 files.
 To download or download a free copy visit:
 Later HDFView binaries require C++ redistributables. If you install the viewer and still cannot access the files, try installing this:
Grain Size Distribution Analysis
 This Excel worksheet calculates statistics for many samples using several methods including Folk and Ward and the Method of Moments.
 Disclaimer: The analysis software GRADISTAT is developed by Kenneth Pyle Associates Ltd. This reference does not imply official or unofficial endorsement.
 Link: http://www.kpal.co.uk/gradistat.html