% 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”.
@ARTICLE{Veglia:610908,
author = {Veglia, Bianca and Agapov, Ilya and Keil, Joachim},
title = {{N}eural {N}etworks for {ID} {G}ap {O}rbit
{D}istortion{C}ompensation in {PETRA} {III}},
journal = {Nuclear instruments $\&$ methods in physics research /
Section A},
volume = {1069},
issn = {0168-9002},
address = {Amsterdam},
publisher = {North-Holland Publ. Co.},
reportid = {PUBDB-2024-04731},
pages = {169934},
year = {2024},
abstract = {Undulators are used in storage rings to produce extremely
brilliant synchrotron radiation. In the ideal case, a
perfectly tuned undulator always has a first and second
field integrals equal to zero. But, in practice, field
integral changes during gap movements can never be avoided
for real-life devices. As they significantly impact the
circulating electron beam, there is the need to routinely
compensate such effects. Deep Neural Networks can be used to
predict the distortion in the closed orbit induced by the
undulator gap variations on the circulating electron beam.
In this contribution several current state-of-the-art deep
learning algorithms were trained on measurements from PETRA
III. The different architecture performances are then
compared to identify the best model for the gap-induced
distortion compensation.},
cin = {MPY},
ddc = {530},
cid = {I:(DE-H253)MPY-20120731},
pnm = {621 - Accelerator Research and Development (POF4-621) / 6G3
- PETRA III (DESY) (POF4-6G3) / ACCLAIM - Accelerating
Science with Artificial Intelligence and Machine Learning
(innovation pool) (ACCLAIM)},
pid = {G:(DE-HGF)POF4-621 / G:(DE-HGF)POF4-6G3 /
G:(DE-Ds200)ACCLAIM},
experiment = {EXP:(DE-H253)PETRAIII(machine)-20150101},
typ = {PUB:(DE-HGF)16},
UT = {WOS:001332686200001},
doi = {10.1016/j.nima.2024.169934},
url = {https://bib-pubdb1.desy.de/record/610908},
}