Re: [Ifeffit] Fitting using Experimental standardAh, I see.  I think Artemis 
has some way of putting in experimental phase and amp, but that may be just to 
make a "corrected" FT.  Is that so?
Otherwise, I suppose it should be possible to write a fake FEFF path file and 
read it in.  I guess that's what you did.
    mam
  ----- Original Message ----- 
  From: Frenkel, Anatoly 
  To: ifeffit@millenia.cars.aps.anl.gov 
  Sent: Monday, January 04, 2010 7:43 PM
  Subject: Re: [Ifeffit] Fitting using Experimental standard


  Thank you, Matthew.
  As they say in Russia, everything new is well forgotten old.
  Seriously, that paper was really how to use FEFFIT for both experimental and 
theoretical standards, not just theoretical.

  A.


  ----- Original Message -----
  From: ifeffit-boun...@millenia.cars.aps.anl.gov 
<ifeffit-boun...@millenia.cars.aps.anl.gov>
  To: XAFS Analysis using Ifeffit <ifeffit@millenia.cars.aps.anl.gov>
  Sent: Mon Jan 04 22:34:56 2010
  Subject: Re: [Ifeffit] Fitting using Experimental standard

  You're describing the way many of us, including me, used to analyze data 
before FEFF became as reliable and easy to use (courtesy of
  Artemis and the like) as it is now.  As shown in the paper,
  you extract amplitude and phase from model compounds, by back-transforming 
filtered shells, then use those to fit data.  Multiple
  data sets aren't new, either; I used to do that with data taken on
  dilute solid solutions at different temperatures.  Another trick I used to 
use a lot was if I didn't have a standard for the right
  pair of atoms, I'd use FEFF to get the difference in scattering factors 
(phase+amp)
  between the pair I wanted and a nearby (in Z) pair I had data for.  For 
instance, you can get CuAl2 as  a compound and extract the
  phase+amp for Cu as the central atom and Al as the scatterer.  You can't do
  that for Cu and Si because there's no Si-rich intermetallic in the CuSi 
system.  Therefore, you can do:

  Amp(Cu->Si) = Amp_exp(Cu->Al)*Amp_Feff(Cu->Si)/Amp_Feff(Cu->Al)
  Phi(Cu->Si) = Phi_exp(Cu->Al)+Phi_Feff(Cu->Si)-Phi_Feff(Cu->Al)

  and get a "semi-empirical" Cu->Si "standard".  Why the +- for phase and the 
*/ for amp?  You can think of it as extrapolating the
  log of a complex signal chi~(k) = Amp(k)*exp(i*Phi(k)), of which the measured 
chi is the Im().
  This expresses everything in terms of relatively slowly-varying quantities 
and treats amp and phi as parts of the same quantity,
  which they really are.

  One of the programs available from the ALS beamline 10.3.2 website 
http://xraysweb.lbl.gov/uxas/Beamline/Software/Software.htm is
  called EXAFSfit and does this sort of fitting to amp and phase.  You feed it 
amp and phases which
  come from the FT program, also available at the website.  The amp and phase 
files are simple 2-column ASCII, thus readable anywhere.
      mam
  ----- Original Message -----
  From: "Frenkel, Anatoly" <fren...@bnl.gov>
  To: "XAFS Analysis using Ifeffit" <ifeffit@millenia.cars.aps.anl.gov>
  Sent: Monday, January 04, 2010 6:21 PM
  Subject: Re: [Ifeffit] Fitting using Experimental standard


  I know of one very obscure conference proceeding describing what you are 
looking for. It was written during pre-Artemis times but
  the method can be used with Artemis, of course.

  A. I. Frenkel, M. Vairavamurthy, and M. Newville,
  A study of the coordination environment in aqueous cadmium-thiol complexes by 
EXAFS spectroscopy: experimental vs. theoretical
  standards
  J. Synchrotron Rad., 8 , 669-771 (2001).

  The link to PDF is here:
  https://pubweb.bnl.gov/~frenkel/EXP-FEFF/thiols.pdf

  Anatoly

  ________________________________

  From: ifeffit-boun...@millenia.cars.aps.anl.gov on behalf of abhijeet gaur
  Sent: Mon 1/4/2010 9:15 AM
  To: ifeffit
  Subject: [Ifeffit] Fitting using Experimental standard


  A very happy new year to all

  Generally the fitting is done using theoretical standards. For that in 
Artemis, we give input as crystallographic data. But If we
  want to use an experimental standard instead of
  theoretical standard, how that can be done. Is it possible to use 
experimental standard in Artemis? or we have to use some other
  method.

  with thanks
  Abhijeet Gaur
  School of Studies in Physics
  Vikram University, Ujjain (India)





  
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