代码搜索:Spectrum

找到约 5,196 项符合「Spectrum」的源代码

代码结果 5,196
www.eeworm.com/read/142092/12963068

m nspabe.m

function [h,xs,w] = nspabe(data,nyy,minw,maxw,t0,t1) % The function NSPABE generates a smoothed and improved HHT spectrum % of data(n,k) in time-frequency space, where % n specifies the lengt
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m nspabd.m

function [h,xs,w] = nspabd(data,nyy,minw,maxw,t0,t1) % The function NSPABD generates a smoothed HHT damping spectrum % in time-frequency space, with fixed frequency range for data(n,k), % where
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m bigd3hilbert.m

echo on; % --- BIGD3HILBERT loads files and plots their 3-D Hilbert spectrum. % Data loaded is 'cp71301'-'cp713100'. % % Non MATLAB Library routines used are: NSPAB, FSPECIAL. % % See marked lin
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m lpcra2pp.m

function pp=lpcra2pp(ra) %LPCAR2PP LPC: Convert ar filter autocorrelation to power spectrum polynomial in cos(w) PP=(RA) % pp is a polynomial such that |polyval(ra,e^jw)| = polyval(pp,cos(w)) %
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m lpcra2pp.m

function pp=lpcra2pp(ra) %LPCAR2PP LPC: Convert ar filter autocorrelation to power spectrum polynomial in cos(w) PP=(RA) % pp is a polynomial such that |polyval(ra,e^jw)| = polyval(pp,cos(w)) %
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m toimage.m

function [im,tt] = toimage(A,f,t,splx,sply) % [im,tt] = TOIMAGE(A,f,t,splx,sply) transforms a spectrum made % of 1D functions (e.g., output of "spectreh") in an 2D image % % inputs : - A : ampli
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m toimage.m

function [im,tt] = toimage(A,f,t,splx,sply) % [im,tt] = TOIMAGE(A,f,t,splx,sply) transforms a spectrum made % of 1D functions (e.g., output of "spectreh") in an 2D image % % inputs : - A : ampli
www.eeworm.com/read/307407/13723394

c evmlogic.c

/* * Copyright (C) 2001, Spectrum Digital, Inc. All Rights Reserved. */ #include "5509.h" #include "util.h" #define LATCH_ADDR ((volatile unsigned *)0x401000) #define FLASH_BASE
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m dmspec.m

function[S,B,B1]=dmspec(L,K,X) % DMSPEC Computes spectrum and bispectrum for discrete wave modes. % % S=DMSPEC(L,K,X), where L is a scalar, K is a array of complex- % valued wavenumbers, X is a
www.eeworm.com/read/304082/13801481

m lpcra2pp.m

function pp=lpcra2pp(ra) %LPCAR2PP LPC: Convert ar filter autocorrelation to power spectrum polynomial in cos(w) PP=(RA) % pp is a polynomial such that |polyval(ra,e^jw)| = polyval(pp,cos(w)) %