NPS Offshore Directional RDI ADCP Data from NCEX Experiment, 2003 Data provided by: Ed Thornton and Tim Stanton Dept of Oceanography Naval Postgraduate School Monterey, CA 93943 thornton@nps.edu, stanton@nps.edu ******************************************************************************* For directional ADCP coordinate location and sampling information, see the file "ncex_locations_nps_metadata.txt" Filename syntaxes: DPSVSpec.tar = tarred, gzipped compilation of all DSpec*.txt, PSpec*.txt, SSpec*.txt, and VSpec*.txt files (described below), to allow easier download of all these files simultaneously. (To uncompress, use "tar xzvf DPSVSpec.tar".) DSpec*.txt = standard output directional spectrum file generated by RDI WAVES software. Matlab loadable. Initial (commented) lines describe number of frequencies and frequency-direction spacing of spectrum. Remaining lines are ordered with rows corresponding to frequency bins and columns corresponding to direction (with first column corresponding to degree value on the last commented line at top, and succeeding columns corresponding to increasing degree values; angles return to zero after passing 360 degrees). Spectral density values are not in standard units. Based on suggestions from RDI, we now use the following conversion algorithms: S(f) = sum(DSpec,2)/(ndir*1e6); S(f,dir) = DSpec/(ndir*1e6*ddir); where S(f) is the frequency spectrum in m^2/Hz, S(f,dir) is the freq-directional spectrum in m^2/(Hz deg), ndir is the total number of directions spaced at ddir, and DSpec contains the originally loaded matrix values. (Note that we are not 100% confident in these algorithms! Use at own risk and contact RDI if clearly erroneous values result.) PSpec*.txt = standard output pressure spectrum file generated by RDI WAVES software. Matlab loadable. Initial (commented) lines provide number and spacing of frequency bands, with modified spectral units. According to RDI, these values may be squared and then multiplied by 1e6 to convert them to m^2/Hz. SSpec*.txt = standard output surface spectrum file generated by RDI WAVES software from echosounder data. Matlab loadable. Initial (commented) lines provide number and spacing of frequency bands, with modified spectral units. According to RDI, these values may be squared and then multiplied by 1e6 to convert them to m^2/Hz. VSpec*.txt = standard output surface spectrum file generated from velocity data by RDI WAVES software. Matlab loadable. Initial (commented) lines provide number and spacing of frequency bands, with modified spectral units. Same conversion method may be applied to convert to m^2/Hz as with PSpec*.txt files. dspec.tar = tarred, gzipped compilation of all dspec*.jpg and dspec*.mat files (described below), to allow easier download of all these files simultaneously. (To uncompress, use "tar xzvf dspec.tar" in unix/linux or WinZip/other compression utility in Windows/Mac.) dspec*.jpg = rough plots of spectral magnitudes from DSpec*.txt files with corresponding date and time in filename. These values are intended to show only RELATIVE spectral magnitudes and distribution over frequency and direction; they have not been converted in the manner described below. Direction axis adjusted so that spectrum runs from -180 to 180 degrees (rather than 0 to 360). dspec*.mat = files containing spectral matrices corresponding to the data in corresponding DSpec*.txt file, together with a vector for frequency (Hz) and a vector for direction (deg). Numbering syntax for [D,P,V]Spec*.txt files: [D,P,V]SpecYYMMDDHHmm.txt YY = two-digit year (03 ==> 2003) MM = month (01-12) DD = date (01-31) HH = hour (00-23) mm = minute (00-59) Times are recorded in Pacific Standard Time, 2003. For further data-related questions, contact Mark Orzech, orzech@nps.edu