% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@MISC{Mller:1031865,
author = {Möller, Sören and Finsterbusch, Martin and Muzakka,
Khoirul Faiq},
title = {{M}e{V} {I}on beam analysis of granite in 10000 points},
publisher = {Zenodo},
reportid = {FZJ-2024-05873},
year = {2024},
abstract = {The dataset presents 10000 ion-beam-analysis (IBA)
measurements of a granite using 2970+-20 keV protons. Figure
1 shows an example of the result. 10,000 points are acquired
in a regular 100x100 point grid with 50 µm beam spot size
and step-size. Four detectors acquire the data
simultaneously for RBS, NRA, PIGE, and PIXE. The description
of the end-station and detectors can be found here:
https://doi.org/10.3390/instruments5010010. Each point on
the sample consists of 4 files, four detector spectra. The
filename consists of the sample name, three positions in
units of nm (X, Y, Z), a rotation in units of µ° followed
by an underscore ( $_$ ) and the type of data contained in
the file (RBS, NRA, PIXE, PIGE, or Meta). Only X and Z
positions are relevant in this case as indicated in the
attached figure. The RBS, NRA, and PIGE detector files
contain a header specifying the dead- and live-time followed
by two columns. The first column represents the digital
channel of the detector. The second column represents the
counts acquired in this channel. This format is readable as
ASCI by SimNRA7. The PIXE file contains the number of
channels in the first row/header and only the counts in the
subsequent rows. The channel is given by the row number.
This format is readable by GUPIXWIN3. The channels of the
detector files can be re-calculated using a calibration
shown in the following table 1. Certain drifts in the
calibrations are possible, but should be limited to below
$2\%$ of the given value. All points are integrated to the
same ion dose of 0.07 µC. This corresponds to a Particle*Sr
of about 5.0E+09 (RBS detector), 5.4E+10 (NRA). RBS Spectra
can be empty or feature a strong low energy background due
to excessive scintillation light. Empty spectra can be
ignored. The background can be mitigated by ignoring
channels},
cin = {IMD-2},
cid = {I:(DE-Juel1)IMD-2-20101013},
pnm = {1222 - Components and Cells (POF4-122)},
pid = {G:(DE-HGF)POF4-1222},
typ = {PUB:(DE-HGF)32},
doi = {10.5281/ZENODO.13944189},
url = {https://juser.fz-juelich.de/record/1031865},
}