- Ifeffit - millenia.cars.aps.anl.gov

Cr(III) adsorbed to or coprecipitated with iron oxides
by Luxton.Todd＠epamail.epa.gov 08 Apr '10

08 Apr '10

I am trying to track down spectra of Cr(III) adsorbed to or coprecipitated with iron oxides. Any data would be great. Thanks Todd Luxton PhD. Post Doctoral Research Soil Scientist U.S. Environmental Protection Agency National Risk Management Research Laboratory Land Remediation and Pollution Control Division 5995 Center Hill Ave. Cincinnati, OH 45224-7879 Luxton.Todd(a)epa.gov Office: (513) 569-7210 Fax: (513) 569-7879

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raw xmu data of fe foil
by Neetu parsai 07 Apr '10

07 Apr '10

Hi, Can anyone give me raw xmu data of fe foil at room temperature that I need for some data analysis. Thanks Mrs.Neetu Parsai Head Department of Engg.Physics Sanghvi Innovative Academy Indore. Residence: 130 Hemu colony, New G.D.C.Road, Indore-452015(M.P.) India.

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No background subtraction in some cases?
by Alexander Riskin 02 Apr '10

02 Apr '10

Dear all, Recently we've measured samples at the DUBBLE Beamline at ESRF for iron and molybdenum (K-edge). After measuring, the DUBBLE software generates a .dat file which must then be translated to other files (depending on the fact whether transmission or fluorescence is measured) using some script in linux. When we try to import some of these transformed files (for transmission measured) into Athena however, the program fails to subtract a background from mu(E), therefore no k and R-space plots are available (see project files MoPEL002 and MoPEL004, the original dat.sample files are included in the zip files). Other files however, work fine (both transmission and fluorescence measured ones). After analyzing the structure of the .dat files, it was discovered which columns are the Io an It data and the correct ln(Io/It) could be manually generated. This manual procedure yields data sets identical to the ones in the dat.sample files, we named them dat.good files. When importing these files into Athena, the background subtraction works fine. It is the exact same data however... Although the problem can be bypassed by processing the data manually, the fact that Athena processes some files correctly and others not seems very strange to us since they all come from the same beamline. We thought it would be interesting to let you all know. Thanks for your time and for making such wonderful software, Alexander Riskin -- Alexander Riskin Universiteit Hasselt IMO - Inorganic and Physical Chemistry Agoralaan – Building D BE-3590 Diepenbeek / Belgium tel. +32.(0)11.26.83.94 fax. +32.(0)11.26.83.23 email: alexander.riskin(a)uhasselt.be

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Fwd: about athena
by Bruce Ravel 30 Mar '10

30 Mar '10

Hi all, Could one of you Mac folks advise Delphine on this issue? B ---------- Forwarded Message ---------- Subject: about athena Date: Tuesday 30 March 2010 From: Delphine Cabaret <delphine.cabaret(a)impmc.jussieu.fr> To: bravel(a)bnl.gov Dear Bruce, How do you do since Camerino ? I would like to install Athena on my Macintosh (MacOS X.6.1). Unfortunately the installation fails from the files copids from the sourceforge. Do you have a version of the program that runs on MaxOS 10.6 ? Thanks for your answer. Best regards delphine -- Delphine Cabaret Maitre de Conferences Université Pierre et Marie Curie (Paris 6) ---------------------------------------------------------------- This message was sent using IMP, the Internet Messaging Program. ------------------------------------------------------- -- Bruce Ravel ----------------------------------- bravel(a)bnl.gov National Institute of Standards and Technology Synchrotron Measurements Group, Beamlines X23A2, X24A, U7A Building 535A, Room M7 Brookhaven National Laboratory Upton NY, 11973, USA My homepage: http://xafs.org/BruceRavel EXAFS software: http://cars9.uchicago.edu/~ravel/software/exafs/

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Call for Papers - 1st North American Core Shell Spectroscopy Conference
by Carlo Segre 29 Mar '10

29 Mar '10

Call for Papers 1st North American Core Shell Spectroscopy Conference to be held jointly with the 59th Denver X-ray Conference 2-6 August 2010 Denver Marriott Tech Center Hotel, Denver, Colorado, U.S.A. The first North American Core Shell Spectroscopy Conference will be held jointly with the 59th Denver X-Ray Conference, 2-6 August 2010. The conference will feature poster sessions as well as oral presentations and students are particularly encouraged to participate with oral presentation submissions. All topics relating to core shell spectroscopy are welcome, including * X-ray Absorption Spectroscopy * X-ray Fluorescence Spectroscopy / Fluorescence Mapping * Resonant Inelastic X-ray Scattering / X-ray Raman Scattering * X-ray Magnetic Circular Dichroism The conference will feature a special session and dinner in honor of Ed Stern. The list of invited speakers for this special session will be posted on the Denver X-ray Conference web site as it is finalized. Participants will be able to attend Denver X-Ray Conference Sessions being held in adjacent rooms. Details of the oral presentation sessions will be posted on the DXC web site as they are available. http://www.dxcicdd.com/default.htm Students will be able to register for a reduced cost, be eligible for special student room rates, and apply for funding to attend the conference. Abstract submissions for oral presentations will be open until April 30 and can be made on the Denver X-Ray Conference web site by selecting the "Submit Abstract for the Joint Meeting with the North American Core Shell Spectroscopy Conference" link on the left side of the page (the 8th button down) or directly at the abstract submission page http://www.dxcicdd.com/cssc/cssc_abstract.asp Visit www.dxcicdd.com<http://www.dxcicdd.com/> or more information or contact: Denise Flaherty, Conference Coordinator ICDD 12 Campus Boulevard Newtown Square, PA 19073 P: 610-325-9814 F: 610-325-9823 E: flaherty(a)icdd.com<mailto:flaherty@icdd.com> WWW.DXCICDD.COM<http://WWW.DXCICDD.COM>

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Re: [Ifeffit] Measuring particle size of metal oxide
by Scott Calvin 28 Mar '10

28 Mar '10

Hi Bill, Sorry for my slow response; I've been swamped. And ironically, the fact that I'm very interested in your topic and wanted to give a good reply slowed me from getting to it! I'm also going to repost your question and my response to the IFEFFIT mailing list, as I think it's of general interest. I think you're missing a key idea concerning this procedure. Both my method and Anatoly Frenkel's method for finding particle size rely on comparing the effective coordination for different paths. I am skeptical of EXAFS determinations of particle size using only one path, as coordination number is hard to tease out from other effects that suppress amplitude (sample quality, disorder, vacancies...). But the relative coordination number of different shells is more reliable. So you should be using more than one path, each with its own r (the absorber-scatterer distance), in order to refine a single value for R, the crystallite radius. If you're using Artemis, this is simple enough to do, as each path has a reff value (which is r in the formula you give), and you can define a guessed parameter R. (To do this right, you need to make sure that the r for multiple-scattering paths is the distance from the absorber to the furthest scatterer, not the half-path length. That means putting the value in "by hand" for those paths, rather than using reff.) (If you want a really quick and dirty method, collect a reference for a bulk standard and for your sample, and multiply the FT of the bulk spectrum by the formula, adjusting R until you get a good match. The quick and dirty method doesn't handle multiple-scattering correctly, and has the usual problem of the fact that even for direct-scattering paths the peaks of the FT are shifted from actual absorber-scatterer distances. But it is model-free, which can be nice in some cases.) By the way, the formula you've cited is derived for spherical particles. If they're kinda sorta spherical, it will still give a decent approximation and fit. But if the particles are needle-shaped or flat plates, then it doesn't work well. You either have to derive another formula, or look at Anatoly's papers, which have addressed a number of common morphologies. So far, everything I've said applies to metals, and you asked about oxides. While most of this also applies to oxides, it's important to realize that the nearest-neighbor oxide paths are not suppressed at all; i.e. the formula doesn't apply until the first metal-metal path (but does apply to metal-oxide paths further out). This is because the surface of such particles is generally comprised of oxygen atoms, and the first scattering shell is thus fully populated no matter how small the particles are. --Scott Calvin Sarah Lawrence College On Mar 8, 2010, at 1:45 PM, bill.schwartz(a)yale.edu wrote: > Hi Scott, > > We met a couple of times at the EXAFS last two EXAFS workshops at > BNL, for relative beginners like me. > > I am attempting to determine the particle size of PdO particles > supported on Alumina (3% PdO/Al2O3). > > I am wondering if I can collect EXAFS data and use the formula in > your 2003 Journal of Applied Physics paper(*) to estimate PdO > particle size: > > N_nano = [1-3/4(r/R)+1/16(r/R)^3]N_bulk > > Here is a little more background: > > PdO particles on metal oxide supports are generally smaller and more > dispersed in comparison to Pd metal on the same support. Also, if > PdO is reduced and then re-oxidized at varying temperatures, the re- > oxidized PdO particle size varies with temperature, with higher > oxidation temperatures resulting in smaller PdO particle size. > > I have prepared a series of samples of 3% PdO/Al2O3, where the PdO > has been been reduced and then re-oxideized at various temperatures, > and I would like to use EXAFS to determine the coordination number > of my various samples. > > A major difference in my planned experiment compared to what you > described in your paper is that you examined nickel metal, while I > am looking at a metal oxide. > > So my current questions are: > > 1) Is the above formula reasonable for determining bulk particle > radius (R) of metal oxides? > > 2) If yes, then what is r, since scattering distance between Pd - > Pd and Pd - O are different? Is it reasonable to average the > distances? > > 3) Can N(nano) be determined by averaging the coordination numbers > for the Pd-Pd and Pd-O paths? > > Any guidance you can provide will be greatly appreciated. > > Sincerely, > > Bill > > (*) Determination of crystallite size in a magnetic nanocomposite > using extended x-ray absorption fine structure > > > > >

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Anharmonic correction (Aaron Slowey)
by grant bunker 26 Mar '10

26 Mar '10

Aaron - There are a couple of things you should watch out for when fitting cumulants. First, you should make sure in the fitting process that the third cumulant C3 doesn't get much more than twice C2^(3/2) (i.e. 2 sigma^3) - values much larger than that are probably unphysical, even if they happen to give you a better fit. Second, the cumulant expansion loses its utility if it doesn't converge quickly enough. It's essentially an expansion in terms of order k*sigma, and if that approaches 1 the higher order cumulants may be large enough that convergence is questionable. If you are lucky and the effective distribution is Gaussian, or most of the variance is due to Gaussian broadening of a skewed distribution, it may converge OK, but that shouldn't be assumed a priori. Grant Bunker http://gbxafs.iit.edu

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Anharmonic correction (Aaron Slowey)
by grant bunker 26 Mar '10

26 Mar '10

When fitting the third cumulant, you should watch out for a couple of things. First, you should make sure in the fitting process that the third cumulant C3 doesn't get much more than twice C2^(3/2) (i.e. 2 sigma^3) - values much larger than that are probably unphysical, even if they happen to give you a better fit. Second, the cumulant expansion loses its utility if it doesn't converge quickly enough. It's essentially an expansion in terms of order k*sigma, and if that approaches 1 the higher order cumulants may be large enough that convergence is questionable. If you are lucky and the effective distribution is Gaussian, or most of the variance is due to Gaussian broadening of a skewed distribution, it may converge OK, but that shouldn't be assumed a priori. Grant Bunker On Mar 26, 2010, at 1:41 PM, ifeffit-request(a)millenia.cars.aps.anl.gov wrote: > Send Ifeffit mailing list submissions to > ifeffit(a)millenia.cars.aps.anl.gov > > To subscribe or unsubscribe via the World Wide Web, visit > http://millenia.cars.aps.anl.gov/mailman/listinfo/ifeffit > or, via email, send a message with subject or body 'help' to > ifeffit-request(a)millenia.cars.aps.anl.gov > > You can reach the person managing the list at > ifeffit-owner(a)millenia.cars.aps.anl.gov > > When replying, please edit your Subject line so it is more specific > than "Re: Contents of Ifeffit digest..." > > > Today's Topics: > > 1. Anharmonic correction (Aaron Slowey) > 2. Re: Anharmonic correction (Scott Calvin) > 3. Re: Anharmonic correction (Frenkel, Anatoly) > > > ---------------------------------------------------------------------- > > Message: 1 > Date: Fri, 26 Mar 2010 10:13:56 -0700 > From: Aaron Slowey <aslowey(a)usgs.gov> > To: ifeffit(a)millenia.cars.aps.anl.gov > Subject: [Ifeffit] Anharmonic correction > Message-ID: <9683660E-9ED8-4DBB-8E26-88586073B0F8(a)usgs.gov> > Content-Type: text/plain; charset="us-ascii" > > Dear XAFS community: > > I am fitting Hg L3-edge EXAFS of what I think are mercury sulfide nanoparticles. I fit Fourier filtered 1st shell Hg-to-Sulfur pair correlations for 5 spectra and obtain interatomic distances (r) that are 0.2 angstroms shorter than a cubic HgS(s) (i.e., metacinnabar) and Hg-to-S coordination numbers (N) that range from 2.6 to 3.0 (compared to N = 4 for metacinnabar). Delta_E0 values are less than a few eV, so I think the r's are not 'incorrect' as far as these preliminary fits are based on harmonic atomic vibrations/Gaussian pair-distribution functions. > > What intrigues me most about these data is that the fitted N's are consistent with the average 1st-shell Hg-S coordinations of 1 to 2 nm HgS clusters obtained by isotropically truncating the metacinnabar crystal lattice. In one case, I can also fit first-nearest Hg neighbors in the first shell, and this N is also consistent with a 1 nm HgS cluster. > > My objective is to scrutinize the tentative conclusion that the mercury sulfides in the samples consist of 1 to 2 nm subunits (within a larger aggregate, as determined by DLS). For instance, while the fitted N's are consistent with nanoclusters, the assumption of a metacinnabar lattice to estimate N of nanoclusters is undermined by the shorter interatomic distances fitted to the data. This got me reading the work of Manceau and Combes from the late 1980s and Frenkel et al. (2001) J. Phys. Chem. B. In Frenkel's paper (p. 12691), they describe that they used a "third cumulant" to account for anharmonic corrections, but I'm not sure how exactly this is implemented. > > It is something that you request in a feff.inp file, or is it a path parameter for IFEFFIT to include in its calculations? > > I am using Artemis on Mac OS X 10.6 (thanks to iXAFS 2.1.1 beta!!) to execute FEFF 7 calculations and fit my data. I noticed parameters called "3rd" and "4th" in the path dialog; is "3rd" the same parameter as, for example, the sigma_sub_i_superscript_(3) term in eqn (2) of Frenkel et al. (2001)? > > Thanks for reading this lengthy note... > > Aaron > > Branch of Regional Research, Water Resources > U.S. Geological Survey > Office (650) 329-5474 > Lab (650) 329-4069 > Fax (650) 329-4463 > 345 Middlefield Road, Mail Stop 466 > Menlo Park, California 94025 > http://profile.usgs.gov/aslowey > >

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Anharmonic correction
by Aaron Slowey 26 Mar '10

26 Mar '10

Dear XAFS community: I am fitting Hg L3-edge EXAFS of what I think are mercury sulfide nanoparticles. I fit Fourier filtered 1st shell Hg-to-Sulfur pair correlations for 5 spectra and obtain interatomic distances (r) that are 0.2 angstroms shorter than a cubic HgS(s) (i.e., metacinnabar) and Hg-to-S coordination numbers (N) that range from 2.6 to 3.0 (compared to N = 4 for metacinnabar). Delta_E0 values are less than a few eV, so I think the r's are not 'incorrect' as far as these preliminary fits are based on harmonic atomic vibrations/Gaussian pair-distribution functions. What intrigues me most about these data is that the fitted N's are consistent with the average 1st-shell Hg-S coordinations of 1 to 2 nm HgS clusters obtained by isotropically truncating the metacinnabar crystal lattice. In one case, I can also fit first-nearest Hg neighbors in the first shell, and this N is also consistent with a 1 nm HgS cluster. My objective is to scrutinize the tentative conclusion that the mercury sulfides in the samples consist of 1 to 2 nm subunits (within a larger aggregate, as determined by DLS). For instance, while the fitted N's are consistent with nanoclusters, the assumption of a metacinnabar lattice to estimate N of nanoclusters is undermined by the shorter interatomic distances fitted to the data. This got me reading the work of Manceau and Combes from the late 1980s and Frenkel et al. (2001) J. Phys. Chem. B. In Frenkel's paper (p. 12691), they describe that they used a "third cumulant" to account for anharmonic corrections, but I'm not sure how exactly this is implemented. It is something that you request in a feff.inp file, or is it a path parameter for IFEFFIT to include in its calculations? I am using Artemis on Mac OS X 10.6 (thanks to iXAFS 2.1.1 beta!!) to execute FEFF 7 calculations and fit my data. I noticed parameters called "3rd" and "4th" in the path dialog; is "3rd" the same parameter as, for example, the sigma_sub_i_superscript_(3) term in eqn (2) of Frenkel et al. (2001)? Thanks for reading this lengthy note... Aaron Branch of Regional Research, Water Resources U.S. Geological Survey Office (650) 329-5474 Lab (650) 329-4069 Fax (650) 329-4463 345 Middlefield Road, Mail Stop 466 Menlo Park, California 94025 http://profile.usgs.gov/aslowey

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Fwd: A problem Using FEFF8
by Bruce Ravel 25 Mar '10

25 Mar '10

Hi all, I am forwarding this email I received about a problem runninng Feff8. Does anyone have any advice for this fellow? B ---------- Forwarded Message ---------- Subject: A problem Using FEFF8 Date: Tuesday 23 March 2010 From: 裘南 <qiun(a)ihep.ac.cn> To: bravel(a)anl.gov Dear Mr. Bruce, My name is QIU Nan, I am a student from Institute of High Energy Physics, Chinese Academy of Science. I encountered a preblem When I calculated O K edge of cerium oxide(CeO2) using FEFF8. FEFF found bad counts: Occupation number in getorb is 4.000 , then FEFF repeated pteration again and again. The attached files are feff.inp I used and log1.dat that FEFF generated. Would you so kind to help me to finish this calculation? Best Wishes! QIU Nan 2010-03-24 ------------------------------------------------------- -- Bruce Ravel ----------------------------------- bravel(a)bnl.gov National Institute of Standards and Technology Synchrotron Measurements Group, Beamlines X23A2, X24A, U7A Building 535A, Room M7 Brookhaven National Laboratory Upton NY, 11973, USA My homepage: http://xafs.org/BruceRavel EXAFS software: http://cars9.uchicago.edu/~ravel/software/exafs/

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