Diamond and the UK new light source Chris Christou, X-band workshop, Cockcroft Institute, 1 st December 2008.

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Presentation transcript:

Diamond and the UK new light source Chris Christou, X-band workshop, Cockcroft Institute, 1 st December 2008

Diamond Light Source Energy3 GeV Circumference561.6 m No. cells24 DBA Symmetry6 Straight sections6 x 8m, 18 x 5m Insertion devices4 x 8m, 18 x 5m Beam current300 mA Emittance (h, v)2.7, 0.03 nm rad Lifetime> 10 h Min. ID gap7 mm Beam size (h, v)123, 6  m Beam divergence (h, v)24, 4  rad (at centre of 5 m ID) nominal, non-zero dispersion lattice

Layout of Diamond Light Source Linac 5Hz, 100 MeV 1nC SB, 3nC MB Booster 158.4m, 5 Hz 6mA max Storage ring 562.6m 3 GeV 300 mA Experimental hall and beamlines All current beamlines within building Next phase includes long beamlines Office building Linac, booster and storage ring are in separate vaults

RF Systems Linac: 3GHz 2 x 5.2m Cu DESY structures 2 x 35MW klystrons bunchers Booster: 500MHz 1 x 5 cell Cu PETRA cavity 1 x 60kW IOT Storage ring: 500MHz 3 x 1 cell Nb Cornell cavities 3 x 300kW IOT complex Cavities from Accel. Amplifiers from Thales

S-band linac 100 MeV 5 Hz repetition rate 2 DESY Type II 5.2 m structures Thales TH2100 klystrons thermionic gun short pulse 1 nC, 1 ns long pulse 3 nC < 1 ms x and y emittance < 50 π.mm.mrad 0.2 ns pulse width 100 ps jitter 0.1% energy variation 0.2% energy spread

12 Insertion Devices Installed BeamlineIDType I02U23In-vacuum I03U21In-vacuum I04U23In-vacuum I06HU64APPLE-II I07U23In-vacuum (not yet operational) I11U22In-vacuum I15SCW3.5 T Superconducting Multipole Wiggler I16U27In-vacuum I18U27In-vacuum I19U22In-vacuum I22U25In-vacuum I24U21In-vacuum 10 x in-vacuum undulators 1 x variable polarization APPLEII device 1 x 3.5T superconducting wiggler

Insertion Devices for Future Beamlines I04.1 (Beamline operation date October 2009) Short, ex-vacuum, permanent magnet device. I07 (Oct. ’09) Cryogenic Permanent Magnet Undulator. I12 (Oct. ’09) Superconducting multipole wiggler, 4.2 T. I20 (Dec. ’09) 2 x hybrid wigglers, W83. I10 (Dec. ’10) 2 x APPLE II devices with fast polarization switching proposed. I13 (Apr. ’11) 2 x in-vac. undulators with “double mini-beta” optics proposed. I09 (Apr. ’11) Helical undulator with “double mini-beta” optics proposed.

Current Machine Status TargetAchieved Energy3 GeV3 GeV Beam current300 mA 300 mA Machine Development 250 mA User Mode Emittance - horizontal 2.7 nm rad2.7 nm rad - vertical 27 pm rad4-50 pm rad ~ 27 pm in User Mode Lifetime at 300 mA> 10 h~ 18 h Min. ID gap7 mm 5-7 mm User Mode, depending on ID Stability< 10% 2.5% (H), 7.5% (V) No feedback of beam size 0.5% (H), 1.7% (V) Feedback, Hz & divergence 0.7% (H), 7.3% (V) Feedback, Hz

User-Mode Operations User operations since January 2007 Most recent run: 250 mA maximum, 2 injections/day 300 mA from Jan. 2009

Top-up for users Operated in top-up mode for users from 28 th to 30 th October 2008 Operation in top-up mode does not increase the frequency of beam trips BS-SR injection efficiency very high Some work required on understanding injection efficiency changes Current user period (from 27 th November) is conducted in top-up mode

Beamtime Statistics (to end Sep.) 2008: 3177h delivered with 95.0% uptime, MTBF = 14.6 h 2007: 3120h delivered with 92.4% uptime, MTBF = 10.0 h

The UK’s New Light Source Project Project to consider the scientific case and develop a conceptual design for a possible next generation light source based on a combination of advanced conventional laser and free-electron laser sources. STFC Daresbury and Rutherford Laboratories Accelerator Science and Technology Centre (ASTeC) Central Laser Facility (CLF) Diamond Light Source John Adams and Cockcroft accelerator institutes Various Universities NLS Progress Official Launch, April 11th 2008 Science Workshops, May 13th – June 19th Draft Science Case published, Sep. 11th Science Case approved by the Physical And Life Science committee of the STFC, Oct. 17th  approval to proceed to the design stage

NLS Desired Baseline Specification High brightness (up to 1012 photons/pulse) Coverage from THz to ~ 1 keV in the fundamental ~ 1 kHz repetition rate with even pulse spacing Capable of smooth tuning across most of the spectral range Pulse durations down to ~ 20 fs Two-colour capability for pump-probe experiments High degree of transverse coherence High degree of longitudinal coherence, at least up to 400 eV Synchronised to short pulse lasers

NLS: normal conducting option DesignDESY structure SLAC structure Length5.2 m3.0 m Shunt impedance 51.5 MΩ/m52 MΩ/m Mode2π/3 Q Filling time740 ns690 ns Number of cells15689 DesignNLC/LCLS structure Length0.6 m Shunt impedance 30 MΩ Mode5π/6 S-band for accelerationX-band for phase space linearisation at input to BC1

Power supplies for normal conducting option KlystronsThalesToshibaSLAC ModelTH2155E3730AXL4 WavebandS-band X-band Frequency2998 MHz2856 MHz11.42 GHz Peak power45 MW50 MW Efficiency44%45%40% Gain54 dB51 dB50 dB Pulse length3.5 µs4 µs1.5 µs Solid state inductive adder-style modulator for S-band offers 1 kHz repetition rate (but limited elsewhere) LCLS X-band modulator

Jitter budget for normal conducting option 3 GeV, 0.2nC, 7kA peak current, 0.7mm.mrad normalised emittance, 0.2% ΔE Beam current and structure voltageAccelerating structure before BC1 Before BC1BC1-BC2After BC2X-bandUnits dE/dV MeV/1% dE/dφ MeV/1° dε nx /dV e mm.mrad/1% dε nx /dφ e mm.mrad/1° dI/dV e kA/1% dI/dφ kA/1°

NLS: superconducting option Possible SRF Linac Parameters for NLS

NLS: superconducting option SRF Module Comparison and NLS Application for 1 GeV option

Upgrade Paths Higher photon energies, ≥ 1.5 keV – additional linac Increased rep. rate, ≥ 10 kHz – VHF/SC gun Longitudinal coherence to ≥ 1 keV – improved seeding sources Shorter pulses, ≤ 1 fs – slicing/single-spike Additional FELs/experimental stations Latest News NLS Project Governing Body agreed on Nov. 19th to proceed with the cw superconducting option. Studies will now concentrate on both the straight and recirculating SC linac options, with 1 keV baseline photon energy.

Thanks to Richard Walker, Peter McIntosh and many others for contributions Thank you – any questions?