% 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”.
@INPROCEEDINGS{Nentwich:607326,
author = {Nentwich, Melanie},
title = {{I}nvestigating different placements of the collimating
mirror for the {PETRA} {IV} beamline {A}pp{A}na{XAS}},
reportid = {PUBDB-2024-01837},
year = {2024},
abstract = {PETRA III stands as a premier storage ring X-ray radiation
source, offering exceptional capabilities for scientific
research. The forthcoming PETRA IV upgrade will further
extend the capabilities, empowering researchers to analyze
intricate processes occurring within catalysts, batteries,
and microchips under realistic operating conditions. The
Applied and Analytical quick X-ray Absorption Spectroscopy
beamline (AppAnaXAFS), will be one of the first operating
beamlines within the second phase of the upgrade, which
focuses on the construction and commissioning of the new
west hall. The scientific scope of this beamline lies on
in-situ and operando analysis of various catalytic processes
for efficient conversion among all kinds of application
areas, like “energy” (distribution and storage of energy
in the form of chemical energy carriers), “green
chemistry” (to close the carbon cycle), “earth $\&$
environment” (bio-catalysis as part of biotechnology), and
“air $\&$ space transportation” (synthetic
fuels).Especially for the quick-EXAFS measurements a source
with a broad and continuous spectrum is favorable, which is
why the use of a 3-pole Wiggler is intended. However, this
Wiggler comes at the cost of high divergence and an imminent
loss of intensity at various “obstacles” along the
beamline, e.g. photon shutters and monochromator. To reduce
this loss as much as possible, the use of a collimating
mirror before the monochromator is desired. Generally,
optical elements like mirrors are placed outside the tunnels
to ensure easy maintenance. For PETRA IV, the placement
closest to the source, but outside the tunnel would be at 42
m. Discussions with the responsible vacuum group revealed a
possible position of collimating mirrors at 22 m within the
tunnel.In order to evaluate the advantages and disadvantages
of the different mirror positions, an extensive x-ray
tracing study was performed, considering not only the mirror
position, but also different geometries (parabolic,
toroidal, bent), lengths, coatings, and two different
Wiggler settings.},
month = {Mar},
date = {2024-03-18},
organization = {Annual Meeting of the German
Crystallographic Society, Bayreuth
(Germany), 18 Mar 2024 - 21 Mar 2024},
cin = {FS-PET-D / FS-PET-S},
cid = {I:(DE-H253)FS-PET-D-20190712 /
I:(DE-H253)FS-PET-S-20190712},
pnm = {631 - Matter – Dynamics, Mechanisms and Control
(POF4-631) / EURIZON - European network for developing new
horizons for RIs (871072)},
pid = {G:(DE-HGF)POF4-631 / G:(EU-Grant)871072},
experiment = {EXP:(DE-H253)P-P23-20150101 / EXP:(DE-H253)P-P65-20150101},
typ = {PUB:(DE-HGF)6},
url = {https://bib-pubdb1.desy.de/record/607326},
}