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SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE to 5 keV is just possible (with no margin) Self-seeding with PMU not possible beyond 4 keV Radiation dose at 1 MHz threatens PMU fields (DK/K ~ 0.01%) SCU can extend photon range toward 8 keV (1 MHz), and beyond, can allow TW peak-power levels (120 Hz), and with much less sensitivity to radiation dose L2- Linac L3-Linac HXU SXU Sec. 21-30 LH BC1 BC2 BC3 D2 D10 m-wall 0.65 m 0.93 m 2.50 m L1 “kicker” LTUH LTUS LCLS-I Linac P e 120 kW P e 120 kW P e 250 kW L u 145 m

SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

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Page 1: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

SCUs for the LCLS-II HXR FELP. Emma, et. al.

July 9, 2014

Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV)SASE to 5 keV is just possible (with no margin)Self-seeding with PMU not possible beyond 4 keVRadiation dose at 1 MHz threatens PMU fields (DK/K ~ 0.01%)SCU can extend photon range toward 8 keV (1 MHz), and beyond, can allow TW peak-power levels (120 Hz), and with much less sensitivity to radiation dose

L2-Linac L3-Linac

HXU

SXU

Sec. 21-30

LH BC1 BC2

BC3

D2

D10

m-wall

0.65 m0.93 m

2.50 mL1

“kicker”LTUH

LTUSLCLS-ILinac

Pe 120 kW

Pe 120 kW

Pe 250 kW Lu 145 m

Page 2: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

PMUNbTi Nb3Sn

g = 5 mm

g = 4 mmg = 4 mm

E = 4.0 GeV (nominal)

145 m

gex,y = 0.40 mmIpk = 1 kAsE = 500 keVb = 16 m20% Lu margin3.4-m seg’s1.0-m breaks1 und. missing1.5 keV low-lim.

magnetic gap is 2.3 mm larger than vac. gap, g

7.6 keV SASE4.8 keV SASE6.8 keV

SASE

lu = 25.6 mm, 18.4 mm, 16.8 mmK = 0.6-2.4, 1.1-3.0, 1.3-3.2B = 0.2-1.0 T, 0.6-1.8 T, 0.8-2.0 T

Page 3: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

PMUNbTi Nb3Sng = 5 mm

g = 4 mmg = 4 mm

E = 4.2 GeV (stretch)

8.2 keV SASE145 m

lu = 25.6 mm, 18.4 mm, 16.8 mm

~7 keV HXRSS limit

gex,y = 0.40 mmIpk = 1 kAsE = 500 keVb = 16 m20% Lu margin3.4-m seg’s1.0-m breaks1 und. missing

magnetic gap is 2.3 mm larger than vac. gap, g

Page 4: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

E = 4.8 GeV (20% upgrade)

10 keVSASE

PMUNbTi

Nb3Sn

g = 5 mm

g = 4 mm

g = 4 mm

145 m

lu = 25.6 mm, 18.4 mm, 16.8 mm

8.3 keV HXRSS limit

magnetic gap is 2.3 mm larger than vac. gap, g

Page 5: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

P (T

W)

z (m)

Add field taper to SCU

TeraWatt Peak Power Possible

C. Emma, C. Pellegrini, Z. Huang

1.2 TW

Nb3Sngm = 7.2 mmge = 0.4 umE = 7.8 GeVf = 120 HzIpk = 4 kA

Page 6: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

Possible SCU Layout in LCLS-II (HXR)

Joel Fuerst, ANL

Page 7: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

Joining Three 1.5-m Magnets into a Single 4.5-m Device

• Magnets conduction cooled through gap separation extrusion

• Gap separation ensures “seamless” core-to-core joint

• Core center channels may be omitted

Page 8: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE
Page 9: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE
Page 10: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE
Page 11: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE
Page 12: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE
Page 13: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE
Page 14: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

End corrector End correctorPhase shifter dipole

Alignment verification quadsand Bx correction

Lb

Lb

Second Field Integral with phase shifter

+k +k

-2k

• Compact phase shifter uses one end corrector from each undulator and one extra dipole magnet in between

• Distance between the undulator cores ~13 cm for this layout (could be reduced if alignment quadrupoles are not necessary)

• Joint sections for Nb3Sn undulator are 4 cm long for each core

Joining Two 1.5-m Segments (13 cm extra)

Page 15: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

Cold Break (quadrupole magnet)Conceptual design of a compact quadrupole magnet at breaks

– Directly attached to undulator cold mass– Integrated quadrupole strength of 4 T (LCLS-II) can be obtained– Independently powered coils can be used for x-field correction

End correctorQuadrupole Magnet

Page 16: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

Vertical Alignment with Alignment Quadrupoles• Use reference quads at each end of ~3-m structure

– Tuning and calibration based on line between magnetic center of two quads

– Fiducialization performed with stretched wire measurement and referenced to fiducials on outside of cryostat

– Allows for beam based alignment by moving cryostat to find center of quads with electron beam

Small Alignment QuadFull Length Quadrupole

Page 17: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

DC Resistive-Wall Wakefield (cold bore & warm)

cold bore

warm boreCu Al

Cu

Al

Page 18: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

Parameter NbTi (ANL) Nb3Sn (LBNL) unitsPhoton Energy (4 GeV) 1.5 - 5.0+ 1.5 - 5.0+ keVUnd. Segment Length ~2 ? ~2 ? mUnd. Break Length (cold) 0.5 - 0.7 0.5 - 0.7 mUnd. System Length 145 145 mMissing Segments (HXRSS) 1-2 1-2 -Number of Segments 54 ? 54 ?Magnetic full gap 6.3 6.3 mmVacuum full gap 4.0 4.0 mmUndulator period 18.4 16.8 mmOn-axis field 0.6 - 1.8 0.8 - 2.0 TK parameter 1.1 - 3.0 1.3 - 3.2 -Cryo Power Required ~250 ~250 W

Undulator Parameters (4 GeV)

Page 19: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

SCU Advantages

• Dramatically improved HXR-FEL performance (~7 keV with SC-Linac & 1-TW with Cu-Linac)

• Orders of magnitude less radiation dose sensitivity (1 MW!)• No mechanical motion (DC power supply drives each

segment)• Less tunnel space required – looks like LCLS-I und. (?)• Can easily be arranged as vertical polarizer (hor. fields)• Cryo-plant (4.5K, 280 W) might serve as injector stand-in at 2K

(7.5M$) – cryo-dist. system not incl. • Might drop 5 linac CM’s (3.4 GeV) and still get 5 keV (Ti or Sn)?• Or drop 10 linac CM’s (2.8 GeV) and still get 4 keV (Sn only)?

Page 20: SCUs for the LCLS-II HXR FEL SCUs for the LCLS-II HXR FEL P. Emma, et. al. July 9, 2014 Hard X-Ray (HXR) FEL for LCLS-II must cover 1-5 keV (4-GeV) SASE

1. What decision criterion should be used to make this technology decision in 2015.

2. What is the impact on the LCLS-II project schedule and what additional

resources are needed to develop production SCUs and install them by the same April 2018 date presently planned for the PMUs?

3. What other subsystems would have to be developed / designed / specified

and become part of the baseline? How would they fit into the facility / tunnel?

4. What other reviews would we have to organize before this could become

baseline? 5. What other assurance would you want as the project director before you

can support the change?

Questions