Bob Von Dreele wrote:
> Dear Mohan,
> Look at the iparm file INST_X3A.PRM in \gsas\examples. That is a typical
> synchrotron iparm file. Important points are that IRAD=0 (non standard
> radiation), LAM2=0 (no Ka2) and POLA=0.95 (typical polarization for
> synchrotron radiation). KRATIO is ignored if LAM2=0.
> Bob Von Dreele
> At 08:52 AM 5/9/00 +0200, you wrote:
> >Hi,
> >
> >I am rather new to this community and have few questions
> >about the use of GSAS to analyze synchrotron data. Since there
> >is no alpha_2 radiation what the instrument file should look like.
> >In all the examples I have seen, the k_ratio has been non-zero.
> >Any help in this matter will be greatly appreciated.
> >
> >Thanks
> >Mohan Menon
> >Post Doc
> >Dept. of Chemistry
> >NTNU, Trondheim, Norway
> >
> >[EMAIL PROTECTED]
Thanks a lot.
Mohan
