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@INPROCEEDINGS{Fogel:582569,
author = {Fogel, Vladimir and Ayvazyan, Valeri and Bellandi, Andrea
and Branlard, Julien and Bousonville, Michael and Butkowski,
Lukasz and Cherepenko, Andrey and Choroba, Stefan and
Diomede, Marco and Eckoldt, Hans-Joerg and Goeller,
Sebastian and Hartung, Jens and Hauberg, Axel and Walker,
Nicholas John and Weinhausen, Timo},
title = {{O}ptimization of klystron drive signal and {HV} shape to
reduce energy consumption during operation of the {E}uropean
{XFEL}},
address = {[Geneva]},
publisher = {JACoW Publishing},
reportid = {PUBDB-2023-02058},
isbn = {978-3-95450-231-8},
pages = {1806-1808},
year = {2023},
note = {Literaturangaben;},
comment = {[Ebook] IPAC'23 : 14th International Particle Accelerator
Conference, 7-12 May 2023, Venice, Italy : proceedings /
hosting institutions: INFN, Elettra Sincotrone Trieste ,
[Geneva] : JACoW Publishing, [2023],},
booktitle = {[Ebook] IPAC'23 : 14th International
Particle Accelerator Conference, 7-12
May 2023, Venice, Italy : proceedings /
hosting institutions: INFN, Elettra
Sincotrone Trieste , [Geneva] : JACoW
Publishing, [2023],},
abstract = {Currently 26 RF stations are in operation at the European
X-ray Free Electron Laser (XFEL) and all RF stations can
deliver sufficient power to support 600 µs beam pulse with
an energy up to 17 GeV. These beam parameters require a
power consumption of about 4.9 MW for high-power RF. Of
course, the simplest way to save power is to reduce the XFEL
repetition rate, but with some additional work and research,
and without modifying any hardware, we can save the
modulator power, without any impact on the XFEL performance.
To reduce the power, we offer two methods that can be used
together or separately. The first one is to make full use of
the available power of the klys-tron during the rise and
fall time of the HV pulse, and partial use of the available
power during cavity filling by using phase and amplitude
compensation. As a result, we can reduce the length of the
HV pulse, because we fill the cavities with energy earlier.
The second one is to slowly reduce the klystron HV during
flattop. In total we can reduce the power consumption up to
$30\%,$ at the cost of making the low-level RF control more
complicated as it needs to deal with large phase and
amplitude changes. To solve this problem, we propose a new
feature, dynamic output vector correction (OVC). In this
report we will present some of experimental results from the
klystron test stand and from several XFEL RF stations.},
month = {May},
date = {2023-05-07},
organization = {14th International Particle
Accelerator Conference, Venice (Italy),
7 May 2023 - 12 May 2023},
keywords = {Accelerator Physics (Other) /
mc2-photon-sources-and-electron-accelerators - MC2: Photon
Sources and Electron Accelerators (Other) /
mc2-a06-free-electron-lasers - MC2.A06: Free Electron Lasers
(Other)},
cin = {MHF / MPC / MSK},
cid = {I:(DE-H253)MHF-20220923 / I:(DE-H253)MPC-20210120 /
I:(DE-H253)MSK-20120731},
pnm = {621 - Accelerator Research and Development (POF4-621)},
pid = {G:(DE-HGF)POF4-621},
experiment = {EXP:(DE-H253)XFEL(machine)-20150101},
typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
doi = {10.18429/JACoW-IPAC2023-TUPL018},
url = {https://bib-pubdb1.desy.de/record/582569},
}