标签:des style blog http ar io color os sp
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Voicebox: Speech Processing Toolbox for MATLAB |
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ACTIVLEV Measure active speech level as in ITU-T P.56 [LEV,AF,FSO]=(sp,FS,MODE) |
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ACTIVLEVG Measure active speech level robustly [LEV,AF,FSO]=(sp,FS,MODE) |
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ATAN2SC sin and cosine of atan(y/x) [S,C,R,T]=(Y,X) |
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AXISENLARGE - enlarge the axes of a figure (f,h) |
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BARK2FRQ Convert the BARK frequency scale to Hertz FRQ=(BARK) |
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BERK2PROB convert Berksons to probability |
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BITSPREC round values to a specified fixed or floating precision (X,N,MODE) |
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h is the handle of the colorbar, axis or figure |
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CCWARPF Warp cepstral coefficients M=(F,N,S) |
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FRQ2ERB Convert Hertz to Cents frequency scale [C,CR]=(FRQ) |
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CEP2POW convert cepstral means and variances to the power domain |
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CHOOSENK All choices of K elements taken from 1:N [X]=(N,K) |
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CHOOSRNK All choices of K elements taken from 1:N with replacement. [X]=(N,K) |
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make correlogram, |
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DISTCHAR calculates the cosh spectral distance between AR coefficients D=(AR1,AR2,MODE) |
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DISTCHPF calculates the cosh spectral distance between power spectra D=(PF1,PF2,MODE) |
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DISTEUSQ calculate euclidean, squared euclidean or mahanalobis distance D=(X,Y,MODE,W) |
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DISTISAR calculates the Itakura-Saito distance between AR coefficients D=(AR1,AR2,MODE) |
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DISTISPF calculates the Itakura-Saito spectral distance between power spectra D=(PF1,PF2,MODE) |
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DISTITAR calculates the Itakura distance between AR coefficients D=(AR1,AR2,MODE) |
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DISTITPF calculates the Itakura spectral distance between power spectra D=(PF1,PF2,MODE) |
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DITHERQ add dither and quantize [Y,ZF]=(X,M,ZI) |
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Solves the discrete Lyapunov equation AV‘VA‘ - V‘V +BB‘ =0 |
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DUALDIAG Simultaneous diagonalisation of two hermitian matrices [A,D,E]=(W,B) |
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DYPSA Derive glottal closure instances from speech [gci,goi] = (s,fs) |
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ENFRAME split signal up into (overlapping) frames: one per row. [F,T]=(X,WIN,INC) |
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ENTROPY calculates the entropy of discrete and sampled continuous distributions H=(P,DIM,COND,ARG,STEP) |
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ERB2FRQ Convert ERB frequency scale to Hertz FRQ=(ERB) |
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ESTNOISEG - estimate MMSE noise spectrum [x,zo]=(yf,tz,pp) |
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ESTNOISEM - estimate noise spectrum using minimum statistics |
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EWGRPDEL calculates the energy weighted group delay waveform Y=(X,W,M) |
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FIG2EMF save a figure in windows metafile format (H,S,P) |
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FIGBOLDEN embolden, resize and recolour the current figure =(POS,PV,M) |
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FILTBANKM determine matrix for a linear/mel/erb/bark-spaced filterbank [X,MN,MX]=(P,N,FS,FL,FH,W) |
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FILTERBANK appply filterbank to a signal: [y,zo]=(b,a,x,gd) |
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FINISHAT print estimated finish time of a long computation (FRAC,TOL,FMT) |
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FOPENMKD is the same as FOPEN but creates any missing directories [fid,mes]=(fn,pe,mf,en) |
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FRAC2BIN Convert an column vector to binary S=(D,N,M) |
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FRAM2WAV converts frame values to a continuous waveform [W]=(X,TT,MODE) |
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FRQ2BARK Convert Hertz to BARK frequency scale BARK=(FRQ) |
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FRQ2ERB Convert Hertz to Cents frequency scale [C,CR]=(FRQ) |
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FRQ2ERB Convert Hertz to ERB frequency scale ERB=(FRQ) |
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FRQ2ERB Convert Hertz to Mel frequency scale MEL=(FRQ) |
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FRQ2MIDI Convert frequencies to musical note numbers [N,T]=(F) |
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FXPEFAC PEFAC pitch tracker [FX,TT,PV,FV]=(S,FS,TINC,M,PP) |
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FXRAPT RAPT pitch tracker [FX,VUV]=(S,FS) |
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GAMMABANK gammatone filter bank [b,a,fx,bx,gd]=(n,fs,w,fc,bw,ph,k) |
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GAUSPROD calculates a product of gaussians [G,U,K]=(M,C) |
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GAUSSMIX fits a gaussian mixture pdf to a set of data observations [m,v,w,g,f]=(x,c,l,m0,v0,w0,wx) |
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GAUSSMIXD marginal and conditional Gaussian mixture densities |
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GAUSSMIXG global mean, variance and mode of a GMM |
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GAUSSMIXK approximate Kullback-Leibler divergence between two GMMs + derivatives |
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GAUSSMIXM estimate mean and variance of the magnitude of a GMM |
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create a CART tree for gaussmixm |
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GAUSSMIXP calculate probability densities from or plot a Gaussian mixture model |
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GAUSSMIXT Multiply two GMM pdfs |
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GLOTLF Liljencrants-Fant glottal model U=(D,T,P) |
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GLOTROS Rosenberg glottal model U=(D,T,P) |
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GMMPDF calculated the pdf of a mixture of gaussians p=(x,m,v,w) |
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HISTNDIM - generates and/or plots an n-dimensional histogram |
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HOSTIPINFO get host name and internet connection information |
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HUFFMAN calculates a D-ary huffman code [CC,LL]=(P,A) |
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IMAGEHOMOG Apply a homography transformation to an image with bilinear interpolation |
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IMPORTSII calculates the SII importance function per Hz or per Bark Q=(F,M) |
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IRDCT Inverse discrete cosine transform of real data X=(Y,N) |
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IRFFT Inverse fft of a conjugate symmetric spectrum X=(Y,N,D) |
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KMEANS Vector quantisation using K-harmonic means algorithm [X,G,XN,GG]=(D,K,L,E,X0) |
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KMEANLBG Vector quantisation using the Linde-Buzo-Gray algorithm [X,ESQ,J]=(D,K) |
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LAMBDA2XYZ Convert wavelength to XYZ or RGB colour space X=(L,M) |
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LDATRACE Calculates an LDA transform to maximize trace discriminant [a,f,B,W]=(b,w,n,c) |
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LIN2PCMA Convert linear PCM to A-law P=(X,M,S) |
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LIN2PCMU Convert linear to Mu-law PCM P=(X,S) |
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LOGNMPDF calculate pdf of a multivariate lognormal distribution P=(X,M,V) |
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LOGSUM logsum(x,d,k)=log(sum(k.*exp(x),d)) |
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LPCAA2AO LPC: Convert area function to area ratios AO=(AA) |
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LPCAA2DL LPC: Convert area coefficients to dct of log area DL=(AA) |
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LPCAA2RF LPC: Convert vocal tract areas to reflection coefficients RF=(AA) |
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LPCAO2RF LPC: Convert area ratios to reflection coefficients RF=(AO) |
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LPCAR2AM Convert ar coefs to ar coef matrix [AM,EM]=(AR,P) |
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LPCAR2CC LPC: Convert AR filter to complex cepstrum [CC,C0]=(AR,NP) |
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LPCAR2DB LPC: Convert AR coefs to power spectrum in dB DB=(AR) |
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LPCAR2FF LPC: Convert AR coefs to complex spectrum FF=(AR,NP) |
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LPCAR2RF Convert autoregressive coefficients to formant freq+amp+bw [N,F,A,B]=(AR,T) |
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LPCAR2IM Convert AR coefs to impulse response IM=(AR,NP) |
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LPCAR2LS convert ar polynomial to line spectrum pair frequencies LS=(AR) |
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LPCAR2PF Convert AR coefs to power spectrum PF=(AR,NP) |
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LPCAR2PP LPC: Convert ar filter to power spectrum polynomial in cos(w) PP=(AR) |
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LPCAR2RA Convert ar filter to inverse filter autocorrelation coefs. RA=(AR) |
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LPCAR2RF Convert autoregressive coefficients to reflection coefficients AR=(RF) |
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LPCAR2RR Convert autoregressive coefficients to autocorrelation coefficients RR=(AR,P) |
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LPCAR2ZZ Convert ar filter to z-plane poles ZZ=(AR) |
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LPCAUTO performs autocorrelation LPC analysis [AR,E,K]=(S,P,T) |
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LPCBWEXP expand formant bandwidths of LPC filter ARX=(AR,BW) |
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LPCCC2AR Convert complex cepstrum to ar coefficients AR=(CC) |
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LPCCC2PF Extrapolate complex cepstrum C=(CC) |
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LPCCC2DB Convert complex cepstrum to dB power spectrum DB=(CC,NP,NC) |
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LPCCC2FF Convert complex cepstrum to complex spectrum FF=(CC,NP,NC) |
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LPCCC2PF Convert complex cepstrum to power spectrum PF=(CC,NP,NC) |
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LPCCONV(from,to,x,y)->s convert between LPC parameter sets |
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LPCCOVAR performs covariance LPC analysis [AR,E,DC]=(S,P,T) |
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LPCPZ2ZZ LPC: Power spectrum roots to LPC poles ZZ=(CW) |
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LPCDB2PF Convert decibel power spectrum to power spectrum PF=(DB) |
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LPCDL2AA dct of log area to area coefficients AA=(DL) |
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LPCFF2PF Convert complex spectrum to power spectrum PF=(FF) |
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LPCFQ2ZZ Convert frequencies and q factors to z-plane poles ZZ=(F,Q) |
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LPCIFILT Apply inverse filter to speech signal U=(S,AR,T,DC,FADE) |
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LPCIM2AR Convert impulse response to AR coefs AR=(IM) |
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LPCRF2IS Convert inverse sines to reflection coefficients RF=(IS) |
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LPCLA2RF Convert log areas to reflection coefficients RF=(LA) |
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LPCLO2RF Convert log area ratios to reflection coefficients RF=(LO) |
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LPCLS2AR convert line spectrum pair frequencies to ar polynomial AR=(LS) |
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LPCPF2CC Convert power spectrum to complex cepstrum CC=(PF,NP) |
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LPCPF2FF Convert power spectrum to complex spectrum [FF,FO]=(PF,NP,FI) |
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LPCPF2RR convert power spectrum to autocorrelation coefs RR=(PF,P) |
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LPCPP2PZ LPC: Convert power spectrum polynomial in cos(w) to power spectrum zeros CW=(RP) |
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LPCPP2PZ LPC: Convert power spectrum polynomial in cos(w) to power spectrum zeros PZ=(RP) |
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LPCPZ2ZZ LPC: Power spectrum roots to LPC poles ZZ=(PZ) |
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LPCAR2PF Convert AR coefs to power spectrum PF=(RA,NP) |
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LPCAR2PP LPC: Convert ar filter autocorrelation to power spectrum polynomial in cos(w) PP=(RA) |
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generate n random stable polynomials of order p with a minimum pole |
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LPCRF2AA Convert reflection coefficients to area function AA=(RF) |
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LPCRF2AO Convert reflection coefficients to area ratios AO=(RF) |
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LPCRF2AR Convert reflection coefs to autoregressive coefs [AR,ARP,ARU,G]=(RF) |
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LPCRF2IS Convert reflection coefficients to inverse sines IS=(RF) |
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LPCRF2LA Convert reflection coefficients to log areas LA=(RF) |
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LPCRF2LO Convert reflection coefficients to log area ratios LO=(RF) |
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LPCRR2AR convert reflection coefs to autocorrelation coefs [RR,AR]=(RF,P) |
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LPCRR2AM Convert autocorrelation coefs to ar coef matrix [AM,EM]=(RR) |
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LPCRR2AR convert autocorrelation coefs to ar coefs [AR,E]=(RR) |
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LPCSS2ZZ Convert s-place poles to z-plane poles ZZ=(SS) |
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LPCZZ2AR Convert z-place poles to ar coefficients AR=(ZZ) |
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LPCZZ2CC Convert poles to "complex" cepstrum CC=(ZZ,NP) |
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LPCZZ2SS Convert z-place poles to s-plane poles SS=(ZZ) |
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M2HTMLPWD - create html documentation of files in current directory |
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MAXFILT find max of an exponentially weighted sliding window [Y,K,Y0]=(X,F,nn,D,X0) |
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MAXGAUSS determine gaussian approximation to max of a gaussian vector [p,u,v,r]=(m,c,d) |
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AVEPSPEC calculates the mean square transfer function for a filter D=(B,A) |
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MEL2FRQ Convert Mel frequency scale to Hertz FRQ=(MEL) |
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MELBANKM determine matrix for a mel/erb/bark-spaced filterbank [X,MN,MX]=(P,N,FS,FL,FH,W) |
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MELCEPST Calculate the mel cepstrum of a signal C=(S,FS,W,NC,P,N,INC,FL,FH) |
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MIDI2FRQ Convert musical note numbers to frequencies F=(N,S) |
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MINSPANE calculate minimum spanning tree using euclidean distance [p,s]=X |
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MINTRACE find row permutation to minimize the trace p=(x) |
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MODSPECT Calculate the modulation spectrum of a signal C=(S,FS,W,NC,P,N,INC,FL,FH) |
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MOMFILT calculates moments of a signal using a sliding window Y=(X,R,W,M) |
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MOS2PESQ convert MOS speech quality scores to PESQ p=(m) |
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NEARNONZ replace each zero element with the nearest non-zero element [V,Y,W]=nearnonz(X,D) |
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OVERLAPADD join overlapping frames together X=(F,WIN,INC) |
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PCMU2LIN Convert A-law PCM to linear X=(P,M,S) |
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PCMU2LIN Convert Mu-law PCM to linear X=(P,S) |
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PEAK2DQUAD find quadratically-interpolated peak in a 2D array |
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PERMUTES All N! permutations of 1:N + signatures [P,S]=(N) |
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PESQ2MOS convert PESQ speech quality scores to MOS m=(p) |
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PHON2SONE convert PHON loudness values to SONEs s=(p) |
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POLYGONAREA Calculate the area of a polygon |
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POLYGONWIND Test if points are inside a polygon |
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POLYGONXLINE Find where a line crosses a polygon [xc,ec,tc,xy0]=(p,l) |
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POTSBAND Design filter for 300-3400 telephone bandwidth [B,A]=(FS) |
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CEP2POW convert cepstral means and variances to the power domain |
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PROB2BERK convert probability to Berksons |
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PSYCDIGIT measures psychometric function using TIDIGITS stimuli |
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Estimate multiple psychometric functions |
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psycestu estimate unimodal psychometric function |
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Calculate psychometric functions: trial success probability versus SNR |
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QRABS absolute value and normalization of a real quaternions [m,q]=[q1] |
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QRDIVIDE divdes two real quaternions q=[q1,q2] |
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QRDOTDIV divides two real quaternions arrays elementwise q=[x,y] |
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QRDOTMULT multiplies together two real quaternions arrays q=[q1,q2] |
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QRMULT multiplies together two real quaternions matrices q=[q1,q2] |
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QRPERMUTE transpose or permute a quaternion array y=[x,p] |
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PEAK2DQUAD find quadratically-interpolated peak in a N-D array |
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RANDFILT Generate filtered gaussian noise without initial transient |
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RANDISCR Generate discrete random numbers with specified probabiities [X]=(P,N,A) |
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RANDVEC Generate real or complex GMM/lognormal random vectors X=(N,M,C,W,MODE) |
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RDCT Discrete cosine transform of real data Y=(X,N,A,B) |
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READAIF Read a .AIF format sound file [Y,FS,WMODE,FIDX]=(FILENAME,MODE,NMAX,NSKIP) |
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READAU Read a SUN .AU format sound file [Y,FS,H]=(FILENAME) |
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READCNX Read a .CNX format sound file [Y,FS,H]=(FILENAME) |
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READWAV Read a .FLAC format sound file [Y,FS]=(FILENAME,MODE) |
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READHTK read an HTK parameter file [D,FP,DT,TC,T]=(FILE) |
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READSFS Read a .SFS format sound file [Y,FS,HD,FFX]=(FF,TY,SUB,MODE,NMAX,NSKIP,XPATH) |
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READSPH Read a SPHERE/TIMIT format sound file [Y,FS,WRD,PHN,FFX]=(FILENAME,MODE,NMAX,NSKIP) |
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READWAV Read a .WAV format sound file [Y,FS,WMODE,FIDX]=(FILENAME,MODE,NMAX,NSKIP) |
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RECTIFYHOMOG Apply rectifying homographies to an image set |
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RFFT Calculate the DFT of real data Y=(X,N,D) |
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RHARTLEY Calculate the Hartley transform of real data Y=(X,N) |
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RNSUBSET choose k distinct random integers from 1:n M=(K,N) |
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ROTATION Encode and decode rotation matrices |
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ROTQR2AX converts a rotation axis and angle to the corresponding real quaternion |
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ROTEU2QR converts a sequence of Euler angles to a real unit quaternion |
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ROTEU2QR converts a sequence of Euler angles to a real unit quaternion |
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ROTMC2QC converts a matrix of complex quaternion matrices to a matrix of complex quaternion vectors |
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ROTMR2QR converts a matrix of real quaternion matrices to quaternion vectors |
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ROTPL2RO find matrix to rotate in the plane containing u and v r=[u,v,t] |
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ROTQC2MC converts a matrix of complex quaternion vectors to quaternion matrices |
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ROTQC2QR converts a matrix of complex quaternion row vectors into real form |
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ROTQR2AX converts a real quaternion to the corresponding rotation axis and angle |
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ROTQR2EQ converts a real unit quaternion into the corresponding euler angles |
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ROTQR2MR converts a matrix of real quaternion vectors to quaternion matrices |
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ROTQR2QC converts a matrix of real quaternion vectors into complex form |
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ROTQR2RO converts a real quaternion to a 3x3 rotation matrix |
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ROTQRMEAN calculates the mean rotation of a quaternion array [y,s]=[q] |
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ROTQRVEC applies a quaternion rotation ot a vector array y=[q,x] |
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ROTRO2EQ converts a 3x3 rotation matrix into the corresponding euler angles |
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ROTRO2PL find the plane and rotation angle of a rotation matrix [u,v,t]=r |
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ROTRO2QR converts a 3x3 rotation matrix to a real quaternion |
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RSFFT fft of a real symmetric spectrum X=(Y,N) |
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SAPISYNTH text-to-speech synthesize of text string or matrix [X,FS,TXT]=(T,M) |
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Pass input signal X through a schmitt trigger |
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SIGALIGN align a clean reference with a noisy signal [d,g,rr,ss]=(s,r,maxd,m,fs) |
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SKEW3D Convert between a vector and the corresponding skew-symmetric matrix |
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SNRSEG Measure segmental and global SNR [SEG,GLO]=(S,R,FS,M,TF) |
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PHON2SONE convert SONE loudness values to PHONs p=(s) |
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SOUNDSPEED gives the speed of sound, density of air and acoustic impedance as a function of temp & pressure [V,D,Z]=(T,P,M,G) |
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SPECSUB performs speech enhancement using spectral subtraction [SS,ZO]=(S,FSZ,P) |
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SPECSUBM obsolete speech enhancement algorithm - use specsub instead |
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SPGRAMBW Draw spectrogram [T,F,B]=(s,fs,mode,bw,fmax,db,tinc,ann) |
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SPHRHARM forward and inverse spherical harmonic transform |
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SPRINTSI Print X with SI multiplier S=(X,D,W) |
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SSUBMMSE performs speech enhancement using mmse estimate of spectral amplitude or log amplitude [SS,ZO]=(S,FSZ,P) |
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SSUBMMSE performs speech enhancement using mmse estimate of spectral amplitude or log amplitude [SS,ZO]=(S,FSZ,P) |
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STDSPECTRUM Generate standard acoustic/speech spectra in s- or z-domain [B,A,SI,SN]=(S,M,F,N,ZI,BS,AS) |
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STOI2PROB convert STOI to probability |
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TEAGER calculate teager energy waveform Y=(X,D,M) |
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TEXTHVC - write text on graph with specified alignment and colour |
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TILEFIGS tile current figures |
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TXALIGN Find the best alignment of two sets of time markers [KX,KY,N,M,S]=(X,Y,MAXT) |
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UNIXWHICH Search system path for an executable program [F]=(C,E) |
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UPOLYHEDRON calculate uniform polyhedron characteristics |
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USASI generates N samples of USASI noise at sample frequency FS X=(N,FS) |
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V_ADDNOISE Add noise at a chosen SNR [z,p,fso]=(s,fsx,snr,m,nb,fsa) |
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V_CHIMV approximate mean and variance of non-central chi distribution [m,v]=(n,l,s) |
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V_COLORMAP set and plot color map |
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V_FINDPEAKS finds peaks with optional quadratic interpolation [K,V]=(X,M,W) |
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V_KMEANS Vector quantisation using K-means algorithm [X,ESQ,J]=(D,K,X0,L) |
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V_PPMVU calculate PPM, VU or EBU level of an audio signal [V,FX,FX1]=(X,FSX,M) |
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V_RESAMPLE Resample and remove end transients [y,h]=(x,p,q,n,b) |
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Singularity in EGG by Multiscale Analysis (SIGMA) Algorithm |
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WINDINFO window information and figures of merit X=(W,FS) |
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WINDOWS Generate a standard windowing function (TYPE,N,MODE,P) |
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VADSOHN implements a voice activity detector [VS,ZO]=(S,FSZ,M,P) |
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VOICEBOX set global parameters for Voicebox functions Y=(FIELD,VAL) |
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VONMISESPDF Von Mises probability distribution P=(x,m,k) |
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WINENVAR get windows environment variable [D]=(N) |
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WRITEHTK write data in HTK format []=(FILE,D,FP,TC) |
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WRITEWAV Creates .WAV format sound files FIDX=(D,FS,FILENAME,MODE,NSKIP,MASK) |
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XTIXKSI labels the x-axis of a plot using SI multipliers S=(AH) |
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XYZTIXKSI labels an axis of a plot using SI multipliers S=(AX,AH) |
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YTIXKSI labels the y-axis of a plot using SI multipliers S=(AH) |
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ZEROCROS finds the zeros crossings in a signal [T,S]=(X,M)% find zero crossings in a signal |
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ZEROTRIM Remove zero trailing rows and columns Z=(X) |
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ZOOMFFT DFT evaluated over a linear frequency range Y=(X,N,M,S,D) |
标签:des style blog http ar io color os sp
原文地址:http://www.cnblogs.com/daleloogn/p/4168013.html