#!/usr/bin/env python # Part of FSL - FMRIB's Software Library # http://www.fmrib.ox.ac.uk/fsl # fsl@fmrib.ox.ac.uk # # Developed at FMRIB (Oxford Centre for Functional Magnetic Resonance # Imaging of the Brain), Department of Clinical Neurology, Oxford # University, Oxford, UK # # # LICENCE # # FMRIB Software Library, Release 5.0 (c) 2012, The University of # Oxford (the "Software") # # The Software remains the property of the University of Oxford ("the # University"). # # The Software is distributed "AS IS" under this Licence solely for # non-commercial use in the hope that it will be useful, but in order # that the University as a charitable foundation protects its assets for # the benefit of its educational and research purposes, the University # makes clear that no condition is made or to be implied, nor is any # warranty given or to be implied, as to the accuracy of the Software, # or that it will be suitable for any particular purpose or for use # under any specific conditions. 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Contact details are: # innovation@isis.ox.ac.uk quoting reference DE/9564. export LC_NUMERIC=C import sys from sys import argv from commands import getoutput from numpy import * def usage(): print "Usage: " + argv[0] + " " print " " print " First argument is the output matrix which will go from the input image to standard space," print " with the desired linear structure aligned with the y-axis in standard space" print " Second argument is the FLIRT transform from the input image to standard" print " Third argument is the input image (e.g., the .nii.gz file)" print " The remaining arguments are two coordinates in the input image, chosen along the" print " linear structure that is to be aligned with the y-axis" print " All coordinates are in voxel coordinates (in the input image)" print " If the input image is already in standard space then use $FSLDIR/etc/flirtsch/ident.mat" print " as the second argument but still use voxel coordinates (not MNI/mm coords)" print " You can use the output matrix from this script in a simple resampling call to flirt:" print " e.g. flirt -in input_image -ref standard_image -applyxfm -init outputfromhere.mat -out rotated_image" print " You can also use a higher resolution standard image as the -ref in the line above if you want better resolution" sys.exit(1) if len(argv) <= 9: usage() # Load in the necessary info a=loadtxt(argv[2]) alldims=getoutput("$FSLDIR/bin/fslsize "+argv[3]+" -s") listdims=alldims.split() dx=float(listdims[12]) dy=float(listdims[14]) dz=float(listdims[16]) #print [dx,dy,dz] x1=matrix([[dx*float(argv[4])],[dy*float(argv[5])],[dz*float(argv[6])],[1]]) x2=matrix([[dx*float(argv[7])],[dy*float(argv[8])],[dz*float(argv[9])],[1]]) # Calculate the desired rotation v=a*(x2-x1) # get rid of x-component as we are not interested in this vn=matrix([[v[1,0]],[v[2,0]]]) norm=sqrt(vn.T * vn) vn=vn/norm # deal with angles greater than 90 degrees (only aligning undirected lines) if vn[0,0]<0: vn=vn*-1.0 theta=arcsin(vn[1,0]) r=matrix([[1,0,0,0],[0,cos(theta),sin(theta),0],[0,-sin(theta),cos(theta),0],[0,0,0,1]]) newa=r*a # Fix the translation (keep COV in the same place) # The input image space COV is ... sx=float(listdims[2]) sy=float(listdims[4]) sz=float(listdims[6]) #print [sx,sy,sz] incov=matrix([[dx*sx/2.0],[dy*sy/2.0],[dz*sz/2.0],[1]]) # The standard image space *COV* (not origin) is ... stdcov=mat("91;109;91;1"); trans=stdcov-newa*incov newa[0:3,3]+=trans[0:3] # Save out the result savetxt(argv[1],newa,fmt='%14.10f')