代码搜索：Difference
找到约 3,389 项符合「Difference」的源代码
代码结果 3,389
www.eeworm.com/read/452217/7445038
m calcbits.m
function [bits]=calcbits(bounds,precision)
% function [bits]=calcbits(bounds,precision)
% Determine the number of bits to represent a float number to the precision
% provided.
%
% bits - the
www.eeworm.com/read/206731/7456725
m calcbits.m
function [bits]=calcbits(bounds,precision)
% function [bits]=calcbits(bounds,precision)
% Determine the number of bits to represent a float number to the precision
% provided.
%
% bits - the
www.eeworm.com/read/441544/7668888
cpp glc.cpp
/*
** Author: Samuel R. Blackburn
** Internet: wfc@pobox.com
**
** Copyright, 1996-2005, Samuel R. Blackburn
**
** "You can get credit for something or get it done, but not both."
** Dr. Richar
www.eeworm.com/read/441544/7668914
cpp gtd.cpp
/*
** Author: Samuel R. Blackburn
** Internet: wfc@pobox.com
**
** Copyright, 1996-2005, Samuel R. Blackburn
**
** "You can get credit for something or get it done, but not both."
** Dr. Richar
www.eeworm.com/read/441544/7668965
cpp lcd.cpp
/*
** Author: Samuel R. Blackburn
** Internet: wfc@pobox.com
**
** Copyright, 1996-2005, Samuel R. Blackburn
**
** "You can get credit for something or get it done, but not both."
** Dr. Richar
www.eeworm.com/read/439446/7708555
m p2_3.m
% Program P2_3
% Generate the input sequences
clf;
n = 0:40;
a = 2;b = -3;
x1 = cos(2*pi*0.1*n);
x2 = cos(2*pi*0.4*n);
x = a*x1 + b*x2;
num = [2.2403 2.4908 2.2403];
den = [1 -0.4 0.75];
ic = [0 0]; %
www.eeworm.com/read/439446/7708633
m p2_3.m
% Program P2_3
% Generate the input sequences
clf;
n = 0:40;
a = 2;b = -3;
x1 = cos(2*pi*0.1*n);
x2 = cos(2*pi*0.4*n);
x = a*x1 + b*x2;
num = [2.2403 2.4908 2.2403];
den = [1 -0.4 0.75];
ic
www.eeworm.com/read/439446/7708728
m p2_3.m
% Program P2_3
% Generate the input sequences
clf;
n = 0:40;
a = 2;b = -3;
x1 = cos(2*pi*0.1*n);
x2 = cos(2*pi*0.4*n);
x = a*x1 + b*x2;
num = [2.2403 2.4908 2.2403];
den = [1 -0.4 0.75];
ic = [0 0]; %
www.eeworm.com/read/438906/7724755
m ct2lg.m
function [dx,dy,dz]=ct2lg(dX,dY,dZ,lat,lon)
% CT2LG Converts CT coordinates to local geodetic.
% Local origin at lat,lon,h. If astronomic lat,lon
% input, then output is in local astronomic syst
www.eeworm.com/read/438906/7724763
m lg2ct.m
function [dX,dY,dZ]=lg2ct(dx,dy,dz,lat,lon)
% LG2CT Converts local geodetic coordinates to CT.
% Local origin at lat,lon,h. If astronomic lat,lon
% input, then output is in local astronomic syst