Separation Scheme Options in the LCLS-II Modified LTU Lattice Y. Nosochkov LCLS-II Physics Meeting, May 9, 2012
Feb 23, 2016
Separation Scheme Options in the LCLS-II Modified LTU Lattice
Y. Nosochkov
LCLS-II Physics Meeting, May 9, 2012
Y. Nosochkov 2
Goals
5/9/2012
Compare HXR/SXR beam separation schemes in the modified LTU lattice:
1. Horizontal kicker with current sheet septum
versus
2. Vertical kicker with Lambertson septum (less expensive)
Compare the kicker strength, orbit amplitude, number of LTU magnets, R56, I5 (ISR emittance growth)
Y. Nosochkov 3
Full lattice with modified LTU
5/9/2012
LTUBypass
Linac
Undulator
HXR
L0
L1 L2 L3HXRSXR
µ
BC2BC1
gun
DL1 DL211-3 to 14-4 14-7 to 20-4
11-1
sd
sd sd
sd
sd
sd
sd
sd
sz szsz
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Existing design of Lambertson septum for vertical separation scheme
5/9/2012 P. Emma
Dy = 7 mm at septum
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First look at the current sheet septum design for horizontal separation (C. Spencer)
5/9/2012
Assume Dx = 10 mm at septum, B = 2.6 kG, L = 2 m.HXR correction may be required to compensate for residual field.
SXR HXR
More expensive
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diagnosticC1
Long drift to minimize wall interference
Low bx at bends
kick
er
sept
um
5/9/2012
Include the kicker orbit as part of the reference trajectoryAdjust septum and SXR main bend field for correction
LTU SXR lattice for horizontal separation
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sept
um
kick
er
QDL
44BX
42Q
DL45
QDL
46
QDL
43
X = -10 mm at septumOff-axis through QDL44,45,46 and BX42
Horizontal separation orbit from kicker
5/9/2012
Y. Nosochkov 8
LTU SXR lattice for vertical separation
5/9/2012
3 extra cells are included thus making the LTUS longer by 52.8 mSeptum angle is reduced ~30%
C1 diagnosticKick
er-1
Kick
er-1
sept
um
C2 C3 C4
by is reduced, but bx at bends is increased
SXR geometry downstream of LTU may need to be adjusted
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Vertical separation orbit and dispersion
5/9/2012
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Parameters
5/9/2012
X-separation Y-separation
LTU HXR + SXR quads 48 54
LTU HXR + SXR main bends 8 8
LTU HXR R56 (mm) 0.385 0.385
LTU SXR R56 (mm) 1.004 0.497
LTU HXR I5 3.0e-9 7.6e-9
LTU SXR I5 4.1e-9 7.7e-9
Kicker-1 (kGm) at 15 GeV 0.173 0.053
Kicker-2 (kGm) 0 0.071
DC1 (kGm) 0.200 0.182
DC2 (kGm) 0.159* 0.394
DC3 (kGm) 0.326* 0.150
DC4 (kGm) 0.055* 0.207
DgISR = 4 10∙ -8 I5 E∙ ∙ 6 = 0.0035 mm-rad at I5 = 7.7e-9 and 15 GeV
* Part of bend field
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Some comparison
5/9/2012
• Lambertson septum: less expensive, lower R56, one extra kicker
• Current sheet septum: fewer quads in LTU, lower emittance growth, correctors combined with dipoles