Hi Jesse,
Sorry for the trouble. I see the same behavior with your data. What is happening is that the first data point for the "mu_fluo_det0" array (and the "fluo_det0" array, and a few other arrays
too) is NaN. That looks to be the case for most, if not every scan in this file. That is messing up the pr-edge and normalization calculation. Basically, `pre_edge()` is removing the point with the NaN from the normalization array, leaving it one point
short, and the plotting routines then give up trying to plot x and y arrays of different sizes.
We generally try to be tolerant of and handle NaNs, but we are failing in this case. I think we can fix this. I’ve started looking at it and am trying to decide on the best strategy here.
--Matt
From: Ifeffit <ifeffit-bounces@millenia.cars.aps.anl.gov> on behalf of
jesse walters <thegeojesse@gmail.com>
Sent: Wednesday, April 10, 2024 7:22 AM
To: ifeffit@millenia.cars.aps.anl.gov <ifeffit@millenia.cars.aps.anl.gov>
Cc: Francesco Ressico <francesco.ressico2@unibo.it>
Subject: [Ifeffit] Difficulty with normalization of XAS spectra
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Hi all,
I have some spectra collected by a collaborator, Francesco Ressico, a PhD student at Uni Bologna, (see attached .h5 file below) and we are having trouble normalizing the Fe K edge spectra. The data are for serpentine group minerals and
were collected in fluorescence mode. In the attached file, the correct X array value is 'energy_enc', the data type is 'xas', and the y array should be 'mu_fluo_det0'. The spectra are already normalized for the incoming beam energy (although this can also
be done using 'flou_det0/i0'). There are multiple spectra in the file, any one of them can be chosen to test the procedure.
After loading the spectra, I am able to plot the raw spectra correctly (see attached). But when I try to normalize the pre and post edge regions and plot the normalized spectra, the software only gives a blank plot. I have tried changing
the normalization type, polynomial type, range, etc for both the pre and post edge, but nothing seems to work. I also tested different spectra, but with similar results.
Does anyone have suggestions for how these data can be normalized?
The h5 file is too large, so here is a dropbox link
https://www.dropbox.com/scl/fi/d8k5s67vli0mq97ac520y/COR21_79_Xastransect_79_F1_THC.h5?rlkey=33ragg4p6x9rx65t9yvi5kewe&dl=0
Sincerely,
Jesse Walters
--
Jesse B. Walters
Ambizione Fellow
Institut für Geologie
Universität Bern