📄 nb_params.sr
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## @(#)nb_params.sr 1.2 3/28/90 ESI ATT# These parameters determine the characteristics of the "narrow-band" # spectrogram. Parameter specifications take the form# key_word <value># Each line may contain one or several of these pairs. All specifications# except the error diffusion filter are optional and may occur in any order.# All comments and blank lines in this file are optional except the line# preceeding the spatial filter coefficients which begins with an asterisk.# Parameters may be changed with any text editor while waves is running so# that the effects of changes may be readily observed.# duration of the window applied to the time series (ms).# The bandwidth of the analysis is inversely proportional to this.win_size_ms 51.2# type of time weighting (windowing) to use when computing the DFT's# 0 ==> rectangular; 1 ==> Hamming; 2 ==> cos**4; 3 ==> Hanningwindow_type 1# time step between adjacent columns in the spectrogram (ms)# This effects both the time resolution and horizontal magnification.win_step_ms 2# coefficient of the first-order preemphasis filter# A value of -1.0 yields +6dB/oct preemphasis; 0.0 results in no preemphasis.preemp -.7# minimum size of the (radix-2) FFT to use in computing spectra (points)# This is automatically increased as necessary to accommodate the window size.fft_points 512# number of pixels displayed vertically for each frequency sample (pixels)# The vertical size of the display in pixels will thus be# (freq_intrp * fft_points)/2.# This variable (freq_intrp) applies only to spectrograms computed by # an external DSP board -- see also min_spec_height in .wave_profreq_intrp 2# factor by which spectral log-magnitude values are multiplied before display# A value of 1.0 is recommended unless the dynamic range must be limited.ampl_scale 1# a constant subtracted from spectral log-magnitude values before display (dB)# This may be used to adjust for overall signal level, if desired.ampl_offset_db 50# fraction of spectral log-magnitude mean subtracted from spectra for display# Note that this interacts with the ampl_offset_dbagc_ratio .0# name of the program to run on the DSP-32 card for spectrogram computationdsp_prog_name $WAVES_32BIN/dspgm# fraction of spectral variance used to normalize displayed variance# This is best left at 0.0 for now...var_norm 0.0# dimensions of the error-diffusion spatial filter (pixels)# These dimensions are only used for monochrome spectrograms.# For wide-band spectrograms y_dither should be larger than x_dither.# For narrow-band spectrograms x_dither should be >= y_dither.# The number of rows and columns should be odd and >= 3. The coefficients# may have any value. If x_dither and y_dither are specified the filter# coefficients MUST be specified. The COEFFICIENTS MUST IMMEDIATELY FOLLOW# THE LINE STARTING WITH THE ASTERISK AND BE THE LAST ITEMS IN THIS FILE.x_dither 5y_dither 3# coefficients of the error-diffusion spatial filter# The first coefficient in the list is for the lower left corner; the last is# for the upper right corner. Note that the last (y_dither/2) coefficients# are zero and are not used. The middle entry in the last column is the# weighting given to the spectral amplitude being quantized. The other# coefficients are used to weight the quantization errors of surrounding# pixels.* the y_dither by x_dither error-diffusion spatial filter follows0. 1. 0.2. 3. 2.3. 5. 3.4. 7. 4.7. 8. 0.
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