Re: [Ifeffit] Silent Oxygen

2017-04-18 Thread Robert Gordon

Hi Fuxiang,

Further to Bruce's note, I looked at your file. Your model splits the 
nearest oxygens by only 0.01A.

Is that the magnitude of splitting you anticipate?
Are you familiar with the resolution criteria for EXAFS?
(k-range [deltak]) * (R-resolution [deltaR]) ~ pi/2 for identical near 
neighbours

This is also discussed in the archives, e.g.:
http://millenia.cars.aps.anl.gov/pipermail/ifeffit/2007-November/003414.html

Looking at your chi(k), it seems usable, charitably, up to about 8 A-1, 
not to 12 A-1 as your
window suggests you have used. Claims of being able to resolve small 
splittings

with this data will be viewed with skepticism.

-R.

On 4/18/2017 11:34 AM, Bruce Ravel wrote:

On 04/18/2017 11:10 AM, Fuxiang Zhang wrote:

Hi, all,
I am in studying the EXAFS of perovskite and clearly see the split of
the first peak after ion irradiation. It should come from a symmetry
change, so I use a tetragonal model (instead the original cubic) which
contains two independent O sites. However, after running Atoms and
Feff, all paths are contributed by only one O atom and nothing related
to another Oxygen atoms (see attached file). As a result it may
be difficult to get a good fit of the first split Ta-O peaks. I am not
sure if it is true or something wrong.
Thank you very much


A fairly common question here on the mailing list.  This is a 
*feature* of Artemis, not a bug.


http://bruceravel.github.io/demeter/documents/Artemis/extended/fuzzy.html

If you want to /model/ a split in distance, you can drag that path 
into the path list twice and adjust the delta R and amplitude 
parameters accordingly.


B




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Re: [Ifeffit] Silent Oxygen

2017-04-18 Thread Bruce Ravel

On 04/18/2017 11:10 AM, Fuxiang Zhang wrote:

Hi, all,
I am in studying the EXAFS of perovskite and clearly see the split of
the first peak after ion irradiation. It should come from a symmetry
change, so I use a tetragonal model (instead the original cubic) which
contains two independent O sites. However, after running Atoms and
Feff, all paths are contributed by only one O atom and nothing related
to another Oxygen atoms (see attached file). As a result it may
be difficult to get a good fit of the first split Ta-O peaks. I am not
sure if it is true or something wrong.
Thank you very much


A fairly common question here on the mailing list.  This is a *feature* 
of Artemis, not a bug.


http://bruceravel.github.io/demeter/documents/Artemis/extended/fuzzy.html

If you want to /model/ a split in distance, you can drag that path into 
the path list twice and adjust the delta R and amplitude parameters 
accordingly.


B


--
 Bruce Ravel   bra...@bnl.gov

 National Institute of Standards and Technology
 Synchrotron Science Group at NSLS-II
 Building 743, Room 114
 Upton NY, 11973

 Homepage:http://bruceravel.github.io/home/
 Software:https://github.com/bruceravel
 Demeter: http://bruceravel.github.io/demeter/
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Re: [Ifeffit] the shortest possible K-range ,

2017-04-18 Thread Matt Newville
Hi Mahmoud,

On Tue, Apr 18, 2017 at 5:11 AM, Al Humaidi, Mahmoud <
mahmoud.alhuma...@student.uni-siegen.de> wrote:

> Hi ,
>
> I want to ask please what is the shortest k-range one can use for "Forward
> Fourier transform"
>
> in my projects I used:
>
> Spline range k 0.0 - 9.0
> k range in Forward Fourier transform 1.0 - 9.0 A^-1
>

That should be OK, though it will limit the resolution and number of
parameters you can use to model the data.

Starting at k=1 Ang^-1 is often considered to be a bit too low for EXAFS
analysis, as this is generally still in the XANES region where multiple
scattering contributions dominate and where the background subtraction is
more uncertain.   That is, starting a k=2 or 3 Ang^-1 might be a better
choice.



>
> I am trying to reduce the contribution of noise in FT ..
>
>
Well, limiting the k-range does not always reduce the noise in the part of
the signal you care about (R= 1 to 6 Ang).  It can, but just because
k^2*chi(k) looks noisier at high k does not necessarily mean the data is
only noisy in that range.  Mostly the noisiness at high-k implies that the
signal-to-noise ratio is reduced, but that's at least partially because the
signal goes down and may not mean the noise is going up.  OTOH, the
measurements sometimes do get noisier at higher energy.


> the attached project shows nice fit ,,,but high phase shift toward lower R
> value ,,
> any recommendation please I will appreciate ..
> and thank you in advance ,
>
>
I don't understand why your "9%" merge data gets weird when making the
spline go past 10 Ang^-1, but the "3%" ad "5%" merge data looks sort of OK
to me going out to 11 or 12 Ang^-1.   I am not sure the signal is real
If these are merged data, I'd suggest looking at the scan to scan
variations to decide if the data is real.

Hope that helps,

--Matt




> best regards
> Mahmoud AL Humaidi
> 
> -
> *Mahmoud Al Humaidi *
>
> Department of Physics, University of Siegen
> Emmy-Noether-Campus
> Walter-Flex-Str. 3, 57072 Siegen
> Room : B-015
> Tel :  +49 (0)  271 740 3727 <+49%20271%207403727>
> -
>
>
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