Hi Gary,
Thanks for the reply. I tried using VVMean but it doesn't seem to be working properly, gave me the following error
bash-3.2$ VVMean -in abc.df.nii.gz -out temp
Thanks for using DTI-TK. This version will expire in -305 days.
Please visit http://www.nitrc.org/projects/dtitk for the up-to-date version.
inFile = DTI_HN_pop.df.nii.gz
outFile = temp 6NãîîîîîwâBÜõ»»'+.ÄÝ
¸{BtöÜ©©¹#÷eÚÕP\>ë|k=¤°u«ÿ
GVíZ=SZµÿÏÇû¶ÌþÇ
Åih({~¢Ü'ÍaïdzpêK#èr;·ÌH&¤0:1£p÷fÑh~Zƽ ,i,ÆÅòç_,s{ÇÑæu5¥ñܸO`BýãHØÚDî$9=µ¹3P÷É,H!üF·a±¦-1½m¾mËÊ;z®°c==ì)ºeÏÝP>và ÄÈT?uäwï÷:gíá4gºüu&£·oº ãÊ¿®ô°r#j¦íÝ9ÙÛsÏÜYëAÕYn{rj«'l¼>ß±ÞüåÍ_ÞDôð¡õKLJ}wÃ)~=éGc¨?»öøåëzÙ"]®qýæa¡ÌÉÁ\Q aã´
Reading ... ** ERROR (nifti_image_read): failed to find header file for '
Done in 0s
fail to load
There was also no documentation so I could not understand what VVMean does exactly. Does it take an average of the three volumes for each voxel? Does it take the euclidean norm of the vector? I noticed some other VV* tools that seemed useful. Is there a documentation for those?
Also, are the warp fields calculated by DTITK iteroperable in FSL and vice versa? Or, can I use DTITK to warp a scalar image?