OK, I have to put in my US$0.02/e0.02. The phase correction can't mean much
if the scattering atoms are different, which is usually
the case. If the scattering atoms are very heavy, then the phase correction
has a kink in it which could cause strange shapes if applied
to light-atom shells. I've played with this phase correction and amplitude
correction, while I was at it, and not been very impressed.
One place where it might be useful is in the aforementioned case of heavy
and light scatterers. If you use the correction for one of
these, then the corresponding shells sharpen and the other ones blur out, so
you can get a rough idea of who's who. I suspect
this works better if you do the amplitude as well.
A related technique is to use model compounds+FEFF to get 'semi-empirical'
amps and phases which include all the artifacts
of the experiment. Suppose, for instance, that you're looking at Cu in a
matrix of Fe, and you have data for Cu metal but
not for any known Cu->Fe scattering pair. You can synthesize a
'semi-empirical' Cu->Fe phase and amp like this:
phi(Cu->Fe) = phi_exp(Cu->Cu)+(phi_theor(Cu->Fe)-phi_theor(Cu->Cu))
amp(Cu->Fe) = amp_exp(Cu->Cu)*amp_theor(Cu->Fe)/amp_theor(Cu->Cu)
If you don't want to do this for modeling, you can use this method for
comparing two spectra which you think might
be alike except for the central atom, by "correcting" one spectrum with the
difference to make it comparable to the other.
Another aspect to this whole thing is that people are very used to
uncorrected FT's and are aware that you have to add 0.3-0.4A
to the distances. If you show only corrected FT's, I wonder if that will be
satisfying to the audience.
mam
----- Original Message -----
From: "John J. Rehr"
Hi all,
I have read Phase corrected Fourier transforms in Athena manual and now I have a big doubt, ¿phase correction or not in a publication?
I have read also that this correction is different (more complete) in Artemis and I am not sure if I should correct also in Artemis and which path should I use and why.
I saw many papers dealing with EXAFS fits and they showed a "calculated" bond distance, I think it is: d = Reff + deltaR, right?
I also ask for a paper where I can find that deltaE is ok (even for high-Z backscatterers) if deltaE < 10eV.
I have high correlations between ss and SO2, and deltaR and deltaE. I tried different fits but I can not eliminate them, then...is the fit wrong?
Sorry for these easy questions but I am a novice in XAFS.
Thank you very much.
Best regards, JA
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