Progress in the energy upgrade of the Southern European Thomson back-scattering source (STAR)

被引:0
作者
Samsam, S. [1 ]
Serafini, L. [1 ,2 ]
Ruijter, M. [1 ,2 ]
Prelz, F. [1 ,2 ]
Conti, M. Rossetti [1 ,2 ]
Bacci, A. [1 ]
Olivieri, A. [3 ,5 ]
Esposito, A. [4 ]
Faillace, L. [4 ]
Gallo, A. [4 ]
Vannozzi, A. [4 ]
Ghigo, A. [4 ]
Liedl, A. [4 ]
Stella, A. [4 ]
Giannotti, D. [6 ]
Puppin, E. [6 ]
Chiarelli, F. [4 ]
Catuscelli, G. [4 ]
Pellegrino, L. [4 ]
Vescovi, S. [4 ]
Bini, S. [4 ]
机构
[1] INFN, Sez Milano, Via G Celo 16, I-20133 Milan, Italy
[2] INFN LASA, Via Fratelli Cervi 210, I-20090 Segrate, Milano, Italy
[3] INFN, Grp Collegato Cosenza, Arcavacata Rende, I-87036 Cosenza, CS, Italy
[4] INFN, Lab Nazl Frascati, Via Enrico Fermi 54, I-00044 Frascati, Italy
[5] UNICAL, Arcavacata Rende, I-87036 Cosenza, CS, Italy
[6] Politecn Milan, Piazza Leonardo da Vinci 32, I-20133 Milan, Italy
关键词
Facility; Thomson scattering; Compton scattering; X-ray source; Radio frequency; Accelerator; Control system; EPICS;
D O I
10.1016/j.nima.2023.168990
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
The Southern European Thomson back-scattering source for Applied Research (STAR) is a high-energy photon facility located on the campus of the University of Calabria (UniCal). The facility was designed for its first phase to operate with an electron and photon energy up to 85 MeV and 140 keV respectively. For the second phase of the project the energy of the electrons, and thereby the photons, would be increased up to 150 MeV and 350 keV respectively. The Italian Institute for Nuclear Physics (INFN) was awarded the project for installing, testing, and commissioning the energy upgrade of the electron beamline. In this article, we will outline the progress of this upgrade. In particular the completion of the site acceptance test of the RF system and the IT infrastructure combined with the control system software.
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页数:3
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