was mistaken.
I'll make an entry in my to do list to look into that.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne
for the scatterer you are interested in
and use the fourth column of that file.
HTH,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room
community.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1) 630 252 5033
that FEFF8.1 was for XANES, not
EXAFS. What was that
about?
Ummm a high degree of confusion on the part of the referee perhaps?
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT
of the Mac -- all I know is what others have written on the
Ifeffit wiki.
HTH,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
detail.
HTH,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1) 630
AA^-1 and making the k-weight for
background removal equal to 2.
And, of course, what Shelly said about using a standard is an
excellent idea.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
/ifeffit/2006-September/002623.html
Let me know if that does not solve the problem.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room
it is available.
I wanted to get the source tarball out the door for the benefit of Jeff and
the other elves working on the MacTel package. When they smooth out the rough
patches in the MacTel distribution, I'd like them to be using the latest
codes.
Enjoy!
B
--
Bruce Ravel
as of yet since I don't know any Ubuntu developers
yet.
Hey Carlo,
I have been playing around with kubuntu on a couple of my computers.
I was, in fact, going to ask you the next time I saw you if the debian
packages would install under ubuntu.
B
--
Bruce Ravel
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1) 630 252 5033
Argonne IL
on this page:
http://cars9.uchicago.edu/iffwiki/FAQ/HoraeQuestions
are probably directly relevant to your problem.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon
for the various flavors of macs can include the
fix in their next versions of their packages.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room
maybe you want to give it a try on
Linux/Mac first.
Gerrit,
Please take a look at the User Contributions part of this wiki page
http://cars9.uchicago.edu/iffwiki/HoraeSoftware
I'd like to make sure I haven't misrepresented you in any way ;-)
B
--
Bruce Ravel
with links to two excellent
articles in how to communicate with software developers. If you are
interested in how to best help me to understand and solve problems with my
software, please read through those articles and take the authors' suggestions
to heart.
Regards,
B
--
Bruce Ravel
Whoops! I just sent this to Han earlier and meant to send it to the
whole list. Silly me!
B
-- Forwarded Message from Bruce Ravel Bruce Ravel
[EMAIL PROTECTED] --
Subject: Re: Independent data poins in Artemis
Date: Thursday 04 January 2007 14:50
From: Bruce Ravel [EMAIL
is to interact with Feff, it interprets the 5 digit thing
quite strictly.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne
= npts(l___cf.energy)
set l___cf.data = splint(l___cf.eee, rh.flat, l___cf.energy)
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advance Photon Source, Building 433
worked at SSRL since my grad school days, I don't really know
how to do so. Your beamline scientist should be able to help you with
that. Perhaps someone on the list will know the details.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental
opened your project file this morning.
There is certainly some kind of bug in Athena. I'll look into this
situation and post something to the list soon.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E
,
That is an AMAZING piece of detective work. I am floored that you
figured out something so weird and specific. Great job!
I will try to find some time this week to figure out the underlying
cause of the problem and update webatoms.
B
--
Bruce Ravel
changed somewhat since then.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice
and defensible regardless of how you decide to
cast the problem. Reasonable and defensible applied to all the
parameters, not just e0.
Hope that helps,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E
?
2. Is 2.59 Angstrom a reasonable value for an equatorial oxygen
ligand in a uranyl moiety?
It would seem that your fit has quite a few problems beyond the
sigma^2 value. I question whether your parameterization of these
three paths is physically defensible.
B
--
Bruce Ravel
their own data with Artemis.
4. The Ifeffit web site, my home page, and especialy http://xafs.org
are all filled with useful information for the XAS novice. If you
haven't already looked through the resources on those sites, you
really should budget some time to do so.
HTH,
B
--
Bruce
should get
things working on you low mem machine. But be aware that you will run
into memory limitations very quickly in Athena and Artemis. For
instance, with the parameters suggested above, Athena could run out of
memory with as few as 20 or 30 groups in the group list.
HTH,
B
--
Bruce Ravel
5.79450
-4.30717-3.84760-0.710294 C43 5.81895
-2.66211-4.25879-2.961644 C37 5.83056
-3.21187 1.06944-4.834734 C25 5.90207
-5.89830-0.63676-0.389294 C13 5.94533
END
--
Bruce Ravel
-- screenshots, transcriptions of error messages, something
that gives a clue as to what the problem is -- someone may be able to
make a useful suggestion.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203
than the number.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1
parameters which are not listed on the path page, are obscure and are
not often used. dphase is useful to people analyzing DAFS data and
the three array valued path parameters definately fall in the catagory
of intended for experts.
--
Bruce Ravel
the filtered specutm a path contribution.
HTH,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory
to know is to try both and see. Hopefully,
Athena does a good job of allowing you to try looking at your data in
several different ways quickly and efficiently.
HTH,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group
a private email and I will do so.
In any event, please do not be mad at those of us who administer the
wiki. We really intend the ifeffit wiki to be a place where you can
bring your children to learn about XAS ;-)
B
--
Bruce Ravel -- [EMAIL PROTECTED
for your own work with IfeffitArtemis.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone
that sigma^2 for the In-P bond be the
same in the amorphous material as in the crystal. Did you measure
crystalline InP as well?
Hope that helps,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1) 630 252 5033
Argonne IL
in quadrature as *the* restraint, not as an argument of the
penalty function.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advance Photon Source, Building 433, Room B007
bugging you, make a suggestion for how you think Athena should
work and I'll consider implementing it.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source
.
The change group label seems to only work for a single group.
Similarly, how to change titles of both Y and X axes within Athena ?
Thanks.
Clement
Edmonton, AB
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group
the next
release.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail
/misc/software.html (may not have a GUI --
it's not clear from the web page)
http://www.download.com/Unix2DOS/3000-2381_4-10488165.html
http://ccrma-www.stanford.edu/~craig/utility/flip/
The last one is probably the one I'd choose, but it may not have a
gui. Still...
HTH,
B
--
Bruce
will work on the next release of
the codes. I have a long list of bugs fixes and improvements that I
hope to roll out for all platforms before the APS XAFS summer school
in July.
Regards,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental
summary is generated on the fly from the raw
file.)
I think that the best work-around would be to rerun the fit when you
open the project on your linux machine. Kind of lame ... I know.
This is on my list of bugs for the next release, which I will be
working on soon.
B
--
Bruce Ravel
button when you first open the project on a unix
machine.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advance Photon Source, Building 433, Room B007
Argonne National
interface without adding much value to its intended user.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National
://millenia.cars.aps.anl.gov/pipermail/ifeffit/2007-March/thread.html
One of the first threads should answer your question. Mark Jensen's
posts are the most useful ones.
If you still have trouble, ask again.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental
becomes invalid
when you change the details of the fitting model is just silly.
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1) 630 252 5033
Argonne IL
From: Moneeb Shatnawi [EMAIL PROTECTED]
To: Bruce Ravel [EMAIL PROTECTED]
Dear Dr. Ravel,
Hello,
I am Moneeb Shatnawi from physics department at Michigan State University,
I have a PDF and XAFS data on GeSe system, and I would like to check if
the PDF and XAFS results are consistent with each
generated for the first few
coordination shells?
B
Feng
EM group, NINT
11421 Saskatachewan Drive
Edmonton, Canada T6G 2M9
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building
' quick first shell theory utility certainly provides you withj
a *very* simple mided model) but a rather sophisticated model to
interpret the PDF, then I suspect it will be very hard indeed to
relate the parameters of the distributions in a physically meaningful
way.
B
--
Bruce Ravel
got the libpgplot5 package
installed...
... may anyone help me, please?
Thanks,
E. Fonda
SAMBA beamline
SOLEIL synchrotron
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10
not
interested in the gifeffit itself, but in the python wrapper. I will test
C. Segre packages if they fix the issue. Thanks, Emiliano.
Is there some feature of gifeffit that you cannot live without?
B.
--
Bruce Ravel -- [EMAIL PROTECTED
to everyone who helped with
this release.
Regards,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory
direct method of putting chi(k) data into Artemis is to read
it directly from the Athena project file. That is, using the Open
file dialog in Artemis, select the Athena project file and use the
Athena project dialog in Artemis to select your chi(k) data.
Regards,
B
--
Bruce Ravel
can do?
Are there any messages in the console window that appears when you
start Artemis? Can you cut and paste those messages into a file or
send me a screenshot. Without more information as to what is going
on, I am not sure how I can best advise you.
B
--
Bruce Ravel
read file name before loading on Athena program under new
version running.
It is useful for data managing. So, I hope for clean up this problem.
Thank you.
Joji Kuniya
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental
/ifeffit
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1) 630 252
not know for sure) that the only difference between
the windows feff84_300.exe and the normal feff84.exe is the size of
the nclusx parameter.
HTH,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
much about such things :-/
That seems right to me. As a test, you could compare the result on
linux with nclusx=300 to what you ran on windows. If they are the
same then the two are equally right (or equally wrong!).
B
--
Bruce Ravel -- [EMAIL
than from the deb package? Are there any messages
written to the screen when you start the programs from the command
line?
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10
On Thursday 30 August 2007, Jun Lin wrote:
Would you please tell me how to build deb package from source?
Instructions for building and installing from source (rather than via
a deb package) are here:
http://cars9.uchicago.edu/~ravel/software/downloads.html
B
--
Bruce Ravel
needed? (I have, of
course, carefully checked the pre-edge and normalization range).
Nope. The XANES LCF fitting uses the normalized spectra. That is
independent of how the background is removed. Sounds like you are
doing the right thing.
HTH,
B
--
Bruce Ravel
!)
HTH,
B
--
Bruce Ravel -- [EMAIL PROTECTED]
Molecular Environmental Science Group, Building 203, Room E-165
MRCAT, Sector 10, Advanced Photon Source, Building 433, Room B007
Argonne National Laboratory phone and voice mail: (1) 630 252
:
http://leonardo.phys.washington.edu/feff/wiki/index.php?title=RMULTIPLIER
HTH,
B
--
Bruce Ravel --- [EMAIL PROTECTED]
National Institute of Standards and Technology
Building 535A, Room M7
c/o Brookhaven National Laboratory
Upton NY, 11973, USA
My
in the
data files are of different orders of magnitude. Normalizing removes
the effect of gains and other purely empirical details from the
measurements. Also, Feff is calculated such that its wiggles are the
same size as the wiggles in our normalized data.
HTH,
B
--
Bruce Ravel
--
Bruce Ravel --- [EMAIL PROTECTED]
National Institute of Standards and Technology
Building 535A, Room M7
c/o Brookhaven National Laboratory
Upton NY, 11973, USA
My homepage:http://xafs.org/BruceRavel
EXAFS software: http://cars9.uchicago.edu/~ravel
is not possible and your choices are
fluorescence with attenuation or going home. Obviously, fluo with
attenuation is the better choice. ;-)
HTH,
B
--
Bruce Ravel --- [EMAIL PROTECTED]
National Institute of Standards and Technology
Building 535A, Room M7
c/o
that Matthew sent me to http://xafs.org/Tutorials.
It's the fourth link under the XAFS Tutorials and Overviews heading.
B
--
Bruce Ravel --- [EMAIL PROTECTED]
National Institute of Standards and Technology
Building 535A, Room M7
c/o Brookhaven National
running Athena (0.8.054) and Artemis (0.8.011) on a laptop (1.7
GHz Pentium M processor 2 GB RAM) with Windows XP Pro.
Thanks!!
-Richard
--
Richard Mayes
Barnes Group
450/452 Buehler Hall
Department of Chemistry
University of Tennessee
Knoxville, TN 37996
--
Bruce Ravel
analysis considering these MS paths? Are you trying to explore the
effect of bond angles on your XANES calculations?
B
--
Bruce Ravel --- [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Measurements Group, Beamlines X23A2, X24A, U7A
--
Bruce Ravel --- [EMAIL PROTECTED]
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
on barium tantalum oxinitride
relevant: Physical Review B73, p. 184121 (2006).
HTH,
B
--
Bruce Ravel --- [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Measurements Group, Beamlines X23A2, X24A, U7A
Building 535A, Room M7
generous with useful information.
Regards,
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
My homepage:http
with enough information to replicate
the problem on my own computers, I am unlikely to be able to solve it.
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
of selected in this context.)
Selected means highlighted in the paths list, that is, the set of
selected paths is the same as the set that gets plotted.
It's certainly possible that it is misbehaving. I'll look into it.
B
--
Bruce Ravel [EMAIL PROTECTED
, that is) and slightly better in the
afternoon.
I saw email about firewall upgrade at APS last weekend. My guess is
that they still are workingon the problem.
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS
On Thursday 03 January 2008 08:54:37 Bruce Ravel wrote:
In Artemis, look in the Fit menu for Save data + this fit. The
final column in that file is the window function. Apparently, the
window column is not saved by any of the options in the File menu.
Fixing that is now on the to do list
, then you will
need to show me what happens. Without providing enough information
for me to reproduce the problem on my own computer, it is not
reasonable to expect that I can solve a problem.
HTH,
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute
of your
fitting model.
HTH,
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
My homepage:http://xafs.org/BruceRavel
the immediate hurdle.
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
My homepage:http://xafs.org/BruceRavel
EXAFS
my copy of the international tables open in front of me for the
last half hour. The symmetry of that space group does indeed require
what you say. And it provides Andreas with a work-around.
I still think that Atoms should not have failed in that situation,
however.
B
--
Bruce Ravel
-3012
Visit us on the web at http://www.chem.tamu.edu
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Ifeffit@millenia.cars.aps.anl.gov
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--
Bruce Ravel [EMAIL PROTECTED
and install anyway.
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
My homepage:http://xafs.org/BruceRavel
EXAFS
work-around for you is to downgrade Tk to
804.027. You seem like a capable linux user, so I don't feel bad
telling you to do so. ;-) Here's the direct link:
http://search.cpan.org/~ni-s/Tk-804.027/.
Good luck,
B
--
Bruce Ravel [EMAIL PROTECTED]
National
, though, I could be pursuaded
Aimee: You can find the Athena document at:
http://cars9.uchicago.edu/~ravel/software/doc/Athena/html/index.html
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group
.
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
My homepage:http://xafs.org/BruceRavel
EXAFS software: http://cars9
regards
Bindu
Dr.Bindu R.
Visiting Fellow
DCMPMS
Tata Institute of Fundamental Research
Homi Bhabha Road
Colaba
Mumbai-400 005
India
Mobile-919892536830
-
5, 50, 500, 5000 - Store N number of mails in your inbox. Click here.
--
Bruce Ravel
correlated with the fit results. Do
you need a better feff or a better background removal? It seems like
a tough question to answer generally.
HTH,
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods
, Marcus knows what he's talking
about.
I was going to guess crappy data analysis software, but that's
always my first answer! ;-)
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS
background removal for that group in order to speed up data processing
and plotting. You can enable normal data processing as Bhoopesh
suggested or by using the dialog described on those two document
pages.
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute
On Friday 18 April 2008 15:11:08 Matt Newville wrote:
PS: Of course, there might be a new version out before 2032
Now, Matt... Don't go making promises we might not be able to keep!
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute
@millenia.cars.aps.anl.gov
http://millenia.cars.aps.anl.gov/mailman/listinfo/ifeffit
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Hi everyone,
I have just spent a fruitless half hour with google scholar trying to
find a paper that publishes Fe L2,3 edge spectra (not K -- I have
those!) of the FeOOH species goethite and lepidocrocite. Can anyone
point me in the right direction? Thanks a million!
B
--
Bruce Ravel
by this opportunity, please let them know.
Sadly, we only have funding for a single scholarship this year, so I
anticipate the competition will be tight.
Regards,
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron
to me directly.
Regards,
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
My homepage:http://xafs.org/BruceRavel
read the papers on mixed ferrites by Scott Calvin or my
paper of BaTaO2N to see how similar problems have been addressed by
the so-called experts on this list.
Hope that helps,
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
My homepage:http://xafs.org/BruceRavel
EXAFS software: http://cars9
On Tuesday 10 June 2008 10:31:06 Carlo Segre wrote:
Hi All:
I am in need of various Ti-O reference spectra. Does anyone have any such
available?
Hey Carlo,
I have various titante perovskites (Eu, Ba, Pb) if those help.
B
--
Bruce Ravel [EMAIL
it entered the rdpadd
subroutine. Recompiling with g77 avoided that problem.
B
--
Bruce Ravel [EMAIL PROTECTED]
National Institute of Standards and Technology
Synchrotron Methods Group at NSLS --- Beamlines U7A, X24A, X23A2
Building 535A
Upton NY, 11973
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