Author: Einfeld, D.
Paper Title Page
TUOAB202 ILSF, A Third Generation Light Source Laboratory in Iran 1137
 
  • J. Rahighi, M.R. Khabazi
    IPM, Tehran, Iran
  • E. Ahmadi, H. Ajam, M. Akbari, S. Amiri, A. Babaei, J. Dehghani, R. Eghbali, J. Etemad Moghadam, S. Fatehi, M. Fereidani, H. Ghasem, A. Gholampour, A. Iraji, M. Jafarzadeh, B. Kamkari, S. Kashani, P. Khodadoost, H. Khosroabadi, M. Moradi, H. Oveisi, S. Pirani, M. Rahimi, M. Razazian, A. Sadeghipanah, F. Saeidi, R. Safian, E. Salimi, Kh.S. Sarhadi, O. Seify, M.Sh. Shafiee, A. Shahveh, A. Shahverdi, D. Shirangi, E.H. Yousefi
    ILSF, Tehran, Iran
  • D. Einfeld
    CELLS-ALBA Synchrotron, Cerdanyola del Vallès, Spain
 
  The Iranian Light Source Facility (ILSF) project is a first large scale accelerator facility which is currently under planning in Iran. The circumference of the storage ring is 297.6 m with the energy of 3 GeV. The facility will be built on a land of 100 hectares area in the city of Qazvin, located 150 km West of Tehran. The city is surrounded by many universities, research centers and industrial companies. The design and construction of prototype items such as radio frequency solid state amplifier, dipole magnets, highly stable magnet power supplies and girders have already begun. A low field H-type dipole magnet with the central field of 0.5T at the gap of 34mm and length of 500mm was built and tested in site. Also a prototype storage ring quadrupole with a 18 T/m gradient and 233 iron length is in now in fabrication process. Site selection studies, including geotechnical and seismological measurements are being performed. Conceptual Design Report, CDR, as the first milestone of the project has been published on October 2012.  
slides icon Slides TUOAB202 [5.173 MB]  
 
MOPEA046 Solaris Project Progress 181
 
  • A.I. Wawrzyniak, C.J. Bocchetta, P.B. Borowiec, D. Einfeld, P.P. Goryl, M. Młynarczyk, R. Nietubyć, M.P. Nowak, W. Soroka, M.J. Stankiewicz, P. Szostak, P.S. Tracz, Ł. Walczak, K. Wawrzyniak, J.J. Wiechecki, M. Zając, Ł. Żytniak
    Solaris, Kraków, Poland
  • D. Einfeld
    MAX-lab, Lund, Sweden
  • R. Nietubyć
    NCBJ, Świerk/Otwock, Poland
 
  Funding: Work supported by the European Regional Development Fund within the frame of the Innovative Economy Operational Program:POIG.02.01.00-12-213/09
Solaris is a 3rd generation light source facility being built in Kraków, Poland at the Jagiellonian University Campus. The project is being accomplished in a tight collaboration with the MAX IV Laboratory in Lund, Sweden. The Solaris 1.5 GeV storage ring is a replica of the MAX IV 1.5 GeV machine, whereas the injector and the transfer line although based on the same components, are unique for Solaris. One of the main differences is the 600 MeV injection energy requiring an energy ramp in the storage ring to the final operating energy of 1.5 GeV. The construction of the facility started in early 2010 and is planned to be finished in the autumn 2014. Up to now, 70% of the components have been procured and construction of the buildings in progress with expected handover in autumn 2013. This paper will give an update on infrastructure progress and design choices for shielding, service area placement of racks and routing of piping and cables. An update is also presented of machine layout that includes the injector, transfer line and storage ring.
 
 
MOPEA047 Ramping of the Solaris Storage Ring Achromat 184
 
  • A.I. Wawrzyniak, C.J. Bocchetta, D. Einfeld, R. Nietubyć
    Solaris, Kraków, Poland
  • D. Einfeld
    MAX-lab, Lund, Sweden
  • R. Nietubyć
    NCBJ, Świerk/Otwock, Poland
 
  Funding: Work supported by the European Regional Development Fund within the frame of the Innovative Economy Operational Program:POIG.02.01.00-12-213/09,
The combined function magnets implemented for the MAX IV and Solaris 1.5 GeV storage ring double bend achromats (DBAs) represents a challenging task in magnetic design. The constituent magnets in the DBA block may be sensitive to saturation effects which must be accounted for, especially in the case of energy ramping, as is the case for Solaris and not for MAXIV, where injection will take place at a beam energy of 0.55-0.6 GeV. The magnetic field distribution was calculated as a function of energy in the range from 0.5 GeV up to 1.5 GeV for the gradient dipole and for the quadrupoles containing a sextupole component. Results show that for the dipole, which generates the strongest field, the relative change of quadrupole strength is lower than 4.10-3. For the quadrupoles the sextupole component is within the relative range of less than 0.7.10-4. The impact on linear and non-linear optics at low energies has been accordingly studied. This is on-going studies and only preliminary results are presented in this paper.
 
 
THPFI043 The Status of the Vacuum System of the MAX IV Laboratory 3382
 
  • E. Al-Dmour, J. Ahlbäck, D. Einfeld, M.J. Grabski, P.F. Tavares
    MAX-lab, Lund, Sweden
  • Ł. Walczak
    Solaris, Kraków, Poland
 
  All the vacuum chambers of the 3 GeV storage ring of MAX IV laboratory are under production. NEG coating R&D has been done to validate technical solutions for the coating process. The standard vacuum chambers for the 1.5 GeV ring of MAX IV and Solaris are designed and they are in the procurement process. We present an update in the technical design of the vacuum chambers following the interaction with the manufacture, the implications on the production due to NEG coating and the design of the vacuum chambers of the 1.5 GeV storage ring.  
 
MOPEA046 Solaris Project Progress 181
 
  • A.I. Wawrzyniak, C.J. Bocchetta, P.B. Borowiec, D. Einfeld, P.P. Goryl, M. Młynarczyk, R. Nietubyć, M.P. Nowak, W. Soroka, M.J. Stankiewicz, P. Szostak, P.S. Tracz, Ł. Walczak, K. Wawrzyniak, J.J. Wiechecki, M. Zając, Ł. Żytniak
    Solaris, Kraków, Poland
  • D. Einfeld
    MAX-lab, Lund, Sweden
  • R. Nietubyć
    NCBJ, Świerk/Otwock, Poland
 
  Funding: Work supported by the European Regional Development Fund within the frame of the Innovative Economy Operational Program:POIG.02.01.00-12-213/09
Solaris is a 3rd generation light source facility being built in Kraków, Poland at the Jagiellonian University Campus. The project is being accomplished in a tight collaboration with the MAX IV Laboratory in Lund, Sweden. The Solaris 1.5 GeV storage ring is a replica of the MAX IV 1.5 GeV machine, whereas the injector and the transfer line although based on the same components, are unique for Solaris. One of the main differences is the 600 MeV injection energy requiring an energy ramp in the storage ring to the final operating energy of 1.5 GeV. The construction of the facility started in early 2010 and is planned to be finished in the autumn 2014. Up to now, 70% of the components have been procured and construction of the buildings in progress with expected handover in autumn 2013. This paper will give an update on infrastructure progress and design choices for shielding, service area placement of racks and routing of piping and cables. An update is also presented of machine layout that includes the injector, transfer line and storage ring.
 
 
MOPEA047 Ramping of the Solaris Storage Ring Achromat 184
 
  • A.I. Wawrzyniak, C.J. Bocchetta, D. Einfeld, R. Nietubyć
    Solaris, Kraków, Poland
  • D. Einfeld
    MAX-lab, Lund, Sweden
  • R. Nietubyć
    NCBJ, Świerk/Otwock, Poland
 
  Funding: Work supported by the European Regional Development Fund within the frame of the Innovative Economy Operational Program:POIG.02.01.00-12-213/09,
The combined function magnets implemented for the MAX IV and Solaris 1.5 GeV storage ring double bend achromats (DBAs) represents a challenging task in magnetic design. The constituent magnets in the DBA block may be sensitive to saturation effects which must be accounted for, especially in the case of energy ramping, as is the case for Solaris and not for MAXIV, where injection will take place at a beam energy of 0.55-0.6 GeV. The magnetic field distribution was calculated as a function of energy in the range from 0.5 GeV up to 1.5 GeV for the gradient dipole and for the quadrupoles containing a sextupole component. Results show that for the dipole, which generates the strongest field, the relative change of quadrupole strength is lower than 4.10-3. For the quadrupoles the sextupole component is within the relative range of less than 0.7.10-4. The impact on linear and non-linear optics at low energies has been accordingly studied. This is on-going studies and only preliminary results are presented in this paper.