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BINP superconducting insertion devices and their applications

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1 BINP superconducting insertion devices and their applications
A.V. Bragin, S.V. Khruschev, N.A. Mezentsev, I.V. Poletaev, V.A. Shkaruba, V.M. Syrovatin, V.M. Tsukanov, A.A. Volkov, E.B. Levichev, S.V. Sinyatkin, K.V. Zolotarev Budker Institute of Nuclear Physics, Novosibirsk, Russia

2 The history of superconductive ID fabrication in the Budker INP
1979 – first in the world 3.5 Tesla superconducting 20 pole wiggler (SCW) for VEPP-3 1984 – 5 pole 8 Tesla superconducting wiggler for VEPP-2 1985 – 4.5 Tesla Superconducting Wave Length Shifter (WLS) for Siberia-1, Moscow 1992 – 6 Tesla Superbend (SB) prototype for compact storage rings Tesla superconducting WLS for PLS, South Korea= T superconducting WLS with fixed point of radiation for CAMD-LSU (USA) 2000 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2000 – 10 Tesla WLS for Spring-8, Japan 2001 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2002 – 3.5 Tesla 49 pole SCW for ELETTRA, Italy 2002 – 7 Tesla 17 pole SCW for BESSY-2, Germany 2004 – 9 Tesla Superbend for BESSY-2, Germany 2005 – 13 Tesla superconducting solenoids for VEPP-2000 2005 – 2 Tesla 63 pole SCW for CLS, Canada 2006 – 3.5 Tesla 49 pole for DLS, England 2006 – 7.5 Tesla 21 pole SCW for Siberia-2, Moscow 2007 – 4.2 Tesla 27 pole SCW for CLS, Canada 2009 – 4.2 Tesla 49 pole SCW for DLS, England 2009 – 4.1 Tesla 35 pole SCW for LNLS, Brasil Tesla 119 pole SCW for ALBA, Spain Tesla SCW for Australian Light Source 2012 – 7.5 Tesla SCW for CAMD-LSU (USA) SCW for ANKA SCW for ANKA & CLIC with indirect cooling 2013 – 2 SCW for Siberia-2, BINP K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

3 The history of superconductive ID fabrication in the Budker INP
1979 – first in the world 3.5 Tesla superconducting 20 pole wiggler (SCW) for VEPP-3 1984 – 5 pole 8 Tesla superconducting wiggler for VEPP-2 1985 – 4.5 Tesla Superconducting Wave Length Shifter (WLS) for Siberia-1, Moscow 1992 – 6 Tesla Superbend (SB) prototype for compact storage rings Tesla superconducting WLS for PLS, South Korea T superconducting WLS with fixed point of radiation for CAMD-LSU (USA) 2000 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2000 – 10 Tesla WLS for Spring-8, Japan 2001 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2002 – 3.5 Tesla 49 pole SCW for ELETTRA, Italy 2002 – 7 Tesla 17 pole SCW for BESSY-2, Germany 2004 – 9 Tesla Superbend for BESSY-2, Germany 2005 – 13 Tesla superconducting solenoids for VEPP-2000 2005 – 2 Tesla 63 pole SCW for CLS, Canada 2006 – 3.5 Tesla 49 pole for DLS, England 2006 – 7.5 Tesla 21 pole SCW for Siberia-2, Moscow 2007 – 4.2 Tesla 27 pole SCW for CLS, Canada 2009 – 4.2 Tesla 49 pole SCW for DLS, England 2009 – 4.1 Tesla 35 pole SCW for LNLS, Brasil Tesla 119 pole SCW for ALBA, Spain Tesla SCW for Australian Light Source 2012 – 7.5 Tesla SCW for CAMD-LSU (USA) SCW for ANKA SCW for ANKA & CLIC with indirect cooling K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

4 K.Zolotarev, Superconductive IDs at BINP, ESLS XXII
Superconducting multipole wigglers BESSY, Germany, 2002 17-poles, 7 Tesla superconducting wiggler ELETTRA, Italy, 2002 49-pole 3.5 Tesla superconducting wiggler CLS, Canada, 2004 63-pole 2 Tesla superconducting wiggler CLS, Canada, 2007 27- poles 4 Tesla Superconducting wiggler DLS, England, 2006 49-pole 3.5 Tesla superconducting wiggler Moscow, Siberia-2, 2007 21-pole 7.5 Tesla superconducting wiggler DLS, England, 2008 49-pole 4.2 Tesla superconducting wiggler LNLS, Brazil, 2009 35-pole 4.2 Tesla superconducting wiggler ALBA, Spain, 2010 119-pole 2.1 Tesla superconducting wiggler K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

5 The history of superconductive ID fabrication in the Budker INP
1979 – first in the world 3.5 Tesla superconducting 20 pole wiggler (SCW) for VEPP-3 1984 – 5 pole 8 Tesla superconducting wiggler for VEPP-2 1985 – 4.5 Tesla Superconducting Wave Length Shifter (WLS) for Siberia-1, Moscow 1992 – 6 Tesla Superbend (SB) prototype for compact storage rings Tesla superconducting WLS for PLS, South Korea T superconducting WLS with fixed point of radiation for CAMD-LSU (USA) 2000 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2000 – 10 Tesla WLS for Spring-8, Japan 2001 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2002 – 3.5 Tesla 49 pole SCW for ELETTRA, Italy 2002 – 7 Tesla 17 pole SCW for BESSY-2, Germany 2004 – 9 Tesla Superbend for BESSY-2, Germany 2005 – 13 Tesla superconducting solenoids for VEPP-2000 2005 – 2 Tesla 63 pole SCW for CLS, Canada 2006 – 3.5 Tesla 49 pole for DLS, England 2006 – 7.5 Tesla 21 pole SCW for Siberia-2, Moscow 2007 – 4.2 Tesla 27 pole SCW for CLS, Canada 2009 – 4.2 Tesla 49 pole SCW for DLS, England 2009 – 4.1 Tesla 35 pole SCW for LNLS, Brasil Tesla 119 pole SCW for ALBA, Spain Tesla SCW for Australian Light Source 2012 – 7.5 Tesla SCW for CAMD-LSU (USA) SCW for ANKA SCW for ANKA & CLIC with indirect cooling Long period SC multipole wigglers (B0 =7-7.5 Tesla, 0~ mm) Medium period SC wigglers (B0 = Tesla, 0~48-60 mm) Short period SC wigglers (B0 =2-2.2 Tesla, 0~30-34 mm) K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

6 Vertical racetrack coils
Resistance of the connection Ohm Advantages of horizontal racetrack coil technology Simplicity of the design Simplicity manufacturing and testing of single coil Lowest inductivity and stored energy Possibility to good thermo stabilization of the coil with using Gd2O2S powder add mixture to the epoxy compound (in wet winding technology) Disadvantage Technology not suitable for mass production of the big number of wigglers (for ex. for CLIC DR) K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

7 Nested coils NbTi CLIC wigler, ALER 2014

8 K.Zolotarev, Superconductive IDs at BINP, ESLS XXII
K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

9 Current lead design NbTi CLIC wigler, ALER 2014

10 Cold mass support structure
Cold mass is hung on Kevlar strings attached to the cold mass support base on one side and to the vacuum vessel on the other. Kevlar strings Vertical support point Vertical support points Horizontal position fixing points Support system: 3 vertical support points; 4 horizontal support points; 4 transport position stoppers Cold mass base frame Transport position keepers K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

11 The history of superconductive ID fabrication in the Budker INP
1979 – first in the world 3.5 Tesla superconducting 20 pole wiggler (SCW) for VEPP-3 1984 – 5 pole 8 Tesla superconducting wiggler for VEPP-2 1985 – 4.5 Tesla Superconducting Wave Length Shifter (WLS) for Siberia-1, Moscow 1992 – 6 Tesla Superbend (SB) prototype for compact storage rings Tesla superconducting WLS for PLS, South Korea T superconducting WLS with fixed point of radiation for CAMD-LSU (USA) 2000 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2000 – 10 Tesla WLS for Spring-8, Japan 2001 – 7 Tesla WLS with fixed radiation point for BESSY-2, Germany 2002 – 3.5 Tesla 49 pole SCW for ELETTRA, Italy 2002 – 7 Tesla 17 pole SCW for BESSY-2, Germany 2004 – 9 Tesla Superbend for BESSY-2, Germany 2005 – 13 Tesla superconducting solenoids for VEPP-2000 2005 – 2 Tesla 63 pole SCW for CLS, Canada 2006 – 3.5 Tesla 49 pole for DLS, England 2006 – 7.5 Tesla 21 pole SCW for Siberia-2, Moscow 2007 – 4.2 Tesla 27 pole SCW for CLS, Canada 2009 – 4.2 Tesla 49 pole SCW for DLS, England 2009 – 4.1 Tesla 35 pole SCW for LNLS, Brasil Tesla 119 pole SCW for ALBA, Spain Tesla SCW for Australian Light Source 2012 – 7.5 Tesla SCW for CAMD-LSU (USA) SCW for ANKA SCW for ANKA & CLIC with indirect cooling K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

12 Indirect cooling conception
LHe vessel SC magnet He fill/vent turret 20 K radiation shield 60 K radiation shield Beam chamber thermal link to cryocooler LHe piping Direct cooled magnet (magnet in bath cryostat) Indirect cooled magnet (magnet in isolation vacuum) Advantages of indirect cooling Easy access to the magnetic system and to the beam vacuum chamber Possibility for exchanging of the elements of magnetic system (and whole system) without complex operation Possibility for exchanging the beam vacuum chamber Possibility for installing of the wigglers in the halls with lower ceilings Effective using of the magnetic gap K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

13 K.Zolotarev, Superconductive IDs at BINP, ESLS XXII
Pole gap and electron beam vertical aperture Indirect cooling magnet Magnet in insulating vacuum Direct cooling magnet with liquid helium (magnet in bath cryostat) Pole gap= V aperture + 4 mm Pole gap = V aperture mm K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

14 K.Zolotarev, Superconductive IDs at BINP, ESLS XXII
CLIC Damping ring K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

15 General view ANKA/CLIC wiggler
Total number of poles 72 Number of main poles 68 Number of additional poles 4 Period 51 mm Magnetic gap 18 mm Peak magnetic field on the main poles 3 T Currents 243 A x4 Stored energy 60 kJ Aperture 13 mm x Additional requirements Possibility for exchanging of the magnetic system in future Possibility for exchanging of the beam vacuum pipe Heating vacuum pipe till 90 K Heating vacuum pipe with power load up to 50 W (with keeping temperature about 40 K) Possibility of activation of the NEG-coating (up to 200o C) K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

16 Heat pipe cooling concept
T = 4 K cooler T = 300 K P = 100 bar LHe Gold coated hemisphere Magnet cooler LHe drops GHe vapor Micro pore material GHe vapor Heat pipes can provide reliable cooling of magnetic system The effective thermo conductivity of He filled pipe (100 bar, room temperature) is about 400 fold higher than for equivalent cupper link LHe Magnet Superconducting magnets for compact heavy ion gantry

17 Nitrogen filled heat pipe
Cryogenic cooler He heat pipe Working range K Evacuation rate 2 W N heat pipe Working range K Evacuation rate 20 W N filed pipe can be operate like a thermal key and can be used for initial fast cooling with using first stage of cryocooler Magnet Superconducting magnets for compact heavy ion gantry

18 Plans and perspectives
Superconducting undulators Horizontal racetrack configuration Period ~ 15 – 18 mm Indirect cooling cryostat Longitudinal gradient dipole magnets A.Wrulich & R.Nagaoka (1992) EMITTANCE MINIMIZATION WITH LONGITUDINAL DIPOLE FIELD VARIATION K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

19 Supercompact high bright hard X-ray light source
Energy E, GeV 1 Damping time Circumference, m 24.3 tx, sec 0.0007 Revolution period, sec 8.11E-08 ty, sec 0.0011 Betatron tunes te, sec qx 3.96 Sigma_s, mm 9.0 qy 0.18 RF voltage 4.59E-01 Emittance, nm*rad 12.1 RF harmonic number 43 Betatron coupling 0.5 % RF frequency, MHz 500 Energy spread 1.40E-03 RF acceptance 2.E-02 Momentum compaction -8.16E-03 Synchrotron tune 4.9E-03 Energy loss, MeV 1.49E-01 Radiation integral Damping partition number I1, m -1.98E-01 Jx 1.53 I2, m^-1 1.06E+01 Jy I3, m^-2 2.07E+01 Je 1.47 I4, m^-1 -5.57E+00 I5, m^-1 1.33E-01 K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

20 Superconducting dipole with longitudinal variation of the field
K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

21 Superconducting dipole for BESSY-II
Vertical aperture, mm Horizontal aperture, mm 30 75 Pole gap, mm 46 Operating magnetic field, T Maximum magnetic field, Т 9.6 Coil material Nb3Sn, NbTi Edge angle, degree 1.3 Current in coil for 8.5 T, A 264 Ramping time 0-7 Tesla, min Ramping time 0-9 Tesla, min <5 <15 Eff. magnetic length along beam, m 0.1777 Bending angle, degree 11.25 Bending radius, m 0.905 Stored energy for 8.5 T, kJ 180 Cold mass, kg 1300 Liquid He consumption ~0.5 l/h K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

22 Thanks for you attention
Acknowledgment A.V. Bragin, S.V. Khruschev, N.A. Mezentsev, E.G. Miginskya, I.V. Poletaev, V.A. Shkaruba, V.M. Syrovatin, V.M. Tsukanov, A.A. Volkov, E.B. Levichev, S.V. Sinyatkin, BINP, Novosibirsk Axel Bernhard, Erhard Huttel, Sara Casalbuoni, Peter Peiffer, Steffen Hillenbrand KIT, Karlsruhe, Daniel Schörling, Paolo Ferracin, Laura Garcia Fajardo CERN Thanks for you attention K.Zolotarev, Superconductive IDs at BINP, ESLS XXII

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