Hi!
I am trying to refine some XRD data using GSAS and looking for an
instrument parameter file for the Rigaku Dmax 2000 x-ray diffractometer.
Can anyone help?
Thanks Donna
Hi!
Just thought i'd quickly introduce myself as I am a new member.
Currently a postdoc researcher in layered oxide materials.
Donna
I don't know the answer to Donna's question but would be interested in
learning how one creates an instrument parameter file for a specific
diffractometer if anyone cares to explain or point me in the direction of
information describing this.
Many thanks to Brian Toby for his space group
A search in the Rietveld archives brings up a wealth of information:
http://pcb4122.univ-lemans.fr/cgi-bin/searchrietveld.pl?Range=AllForma
t=StandardTerms=instrument+parameter+file (old archive)
http://www.mail-archive.com/cgi-bin/htsearch?method=andformat=shortco
Donna (and anyone else who wonders about this),
In gsas\examples there is an iparm file (inst_xry.prm) that can be used for most any
Bragg-Brentano powder diffractometer. These instruments all perform more or less
equally independent of manufacturer with respect to the things of interest for
Your sample will probably broaden the lines (LX, LY, etc.) so much that
any attempt to vary the Gaussian
coefficients will yield nonsense.
Just some remark (of course, I am not a great specialist):
At least to my experience, there is always some Gaussian broadening from
the sample as well, and
At 17:07 18/03/2004, Brian H. Toby wrote:
Please remove me from the mailing list-thank you
I seem to provoke the above response every time I post to the list...
Perhaps :-) But you don't see the requests I have from new people wanting to join,
which seem to increase whenever there is some
Maxim V. Lobanov wrote:
U, V, and W tend to be highly correlated, with a result that various
combinations of quite different values can lead to essentially the
same variance, sigma^2.These three parameters, therefore, do not
converge in a stable manner when refined
U, V, and W tend to be highly correlated
The correlation between U,V,W is the result of a resolution curve that doesn't have a
well defined minimum. If you differentiate the Caglioti equation for the FWHM:
FWHM**2=U.tan**2(theta)+V.tan(theta)+W
you obtain the condition for the minimum as
Theoretically U,V,W should not be refined at all as they describe instrumental
broadening, and this is exactly what I do
(usually). After diffractometer alignment, a good quality pattern in whole possible
angular range has to be collected from Rietveld
standard which currently is LaB6. From
I am going to give up my 'lurker' status on this mailing list to switch
this thread to a more philosophical vein.
In the past generation, many good crystallographers have also been good
programmers. I suspect it was easier to learn programming than it was to
teach crystallography to a
Theoretically U,V,W should not be refined at all as they describe instrumental
broadening
This is true only when there is no Gaussian strain present.
Brian
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