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
www.eeworm.com/read/142092/12963115
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
www.eeworm.com/read/142092/12963510
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
www.eeworm.com/read/320176/13431561
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))
%
www.eeworm.com/read/320175/13431607
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))
%
www.eeworm.com/read/320160/13431896
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/320160/13431903
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
www.eeworm.com/read/305575/13765540
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))
%