📄 ct2lg.m
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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 system.% Vectorized. See also LG2CT.% Version: 18 Jan 96% Useage: [dx,dy,dz]=ct2lg(dX,dY,dZ,lat,lon)% Input: dX - X coordinate difference in CT% dY - Y coordinate difference in CT% dZ - Z coordinate difference in CT% lat - lat of local system origin (rad)% lon - lon of local system origin (rad)% Output: dx - x coordinate in local system (N)% dy - y coordinate in local system (E)% dz - z coordinate in local system (ht)R=zeros(3,3);R(1,1)=-sin(lat).*cos(lon);R(1,2)=-sin(lat).*sin(lon);R(1,3)=cos(lat);R(2,1)=-sin(lon);R(2,2)=cos(lon);R(2,3)=0;R(3,1)=cos(lat).*cos(lon);R(3,2)=cos(lat).*sin(lon);R(3,3)=sin(lat);dx=R(1,:)*[dX';dY';dZ'];dy=R(2,:)*[dX';dY';dZ'];dz=R(3,:)*[dX';dY';dZ'];dx=dx';dy=dy';dz=dz';
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