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The SPEAR3 Upgrade Project at SLAC

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The SPEAR3 Upgrade Project at SLAC. Catherine Le Cocq, Brian Fuss, ... 1 septum magnet. 10/03/2004. IWAA2004. 10. SPEAR3 Beamlines. 3969.94 -108.738 -0.162375 ... – PowerPoint PPT presentation

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Title: The SPEAR3 Upgrade Project at SLAC


1
The SPEAR3 Upgrade Project at SLAC
  • Catherine Le Cocq, Brian Fuss, Michael Gaydosh
  • Alignment Engineering Group
  • SLAC

2
SPEAR History
  • 1972 Commissioning as a 2.4 GeV colliding beam
    facility.
  • 1974 Upgrade to 4 GeV.
  • 1991 Completion of a dedicated electron
    injector.SPEAR2 operates routinely at 2.3 GeV as
    a synchrotron radiation source.
  • IWAA97 Re-Visiting SPEAR After 25 Years poster
    by M. Pietryka and all.
  • 1997 Initial upgrade proposal.
  • 1999 Start of SPEAR3 upgrade project.
  • 2004 3 GeV 100 mA operations.

SLAC-SSRL-SPEAR 3 dedication event of January 29,
2004 The project was completed three months
ahead of schedule, and within its 58M budget.
3
(No Transcript)
4
SPEAR3 Goals
  • 3 GeV injection energy (increase from current 2.3
    GeV).
  • 18 nm-radian beam emittance (reduction from 160
    nm-radian).
  • 100 mA stored beam initially (same as SPEAR 2)
    with future increases towards 500 mA.

5
SPEAR3 Lattice
  • 18 magnet girders
  • 14 standard cells
  • 4 matching cells
  • 18 straight sections
  • 12 are 3.1 m
  • 4 are 4.7 m
  • 2 are 7.6 m
  • 234.126 m storage-ring circumference

6
Standard Cell Part 1
7
Standard Cell Part 2
8
Standard Cell Part 3
9
SPEAR3 Magnets Summary
  • 36 gradient dipoles
  • 28 full-length and 8 3/4 lenghth
  • 94 quadrupoles
  • 4 different lengths 0.60, 0.50, 0.35 and 0.2 m
  • 72 sextupoles
  • 2 different lengths 0.25 and 0.21 m
  • 72 dipole correctors
  • 2 injection dipoles
  • 2 injection quadrupoles
  • 1 septum magnet

10
SPEAR3 Beamlines
The 7 Insertion Devices beamlines stayed in the
same position. The 4 bend magnets beamlines had
to be moved. Here are their SPEAR3
characteristics with respect to the center of the
upstream straight.
11
SPEAR3 Timeline
  • Network 0
  • April SPEAR2 removal
  • May to mid June Floor construction
  • June 13 to 19 New monuments
  • Network 1
  • June 26 July 3 Mark templates
  • Network 2
  • July 18 August 1 Support plates
  • August to November Installation
  • Network 3
  • November 17 to 23 Final alignment
  • December Commissioning
  • 2004 Network

12
Network 0 Description
13
Network 0 Composition
  • Booster TC2002 Survey 9/2001
  • BTS TC2002 Survey 3/2002
  • Building 130 Tracker Survey 7/2002
  • SSRL Tracker Survey 9/2002
  • SPEAR Ring Tracker Survey 11/2002
  • SSRL BL0 TC2002 Survey 2/2003

14
From SPEAR2 To SPEAR3
SPEAR2 Z offset 90000 m X offset 70000 m Y
offset 2000 m H O 0.0 m 22 floor SPxxx3D
SPEAR3 Z offset 6000 m X offset 3000 m
Y offset 500 m H O 75.791 m 38 floor
SMxxFx
15
Network 1
  • Purpose Give values to the new SPEAR3 monuments.
  • Description
  • 166 points
  • 121 ring monuments including 34 new floor and 4
    old floor
  • 45 SSRL and BTS monuments
  • 46 laser tracker stations
  • 611 triplet observations
  • Distances 30 µm
  • Horizontal angles 50 µm / D
  • Vertical angles 50 µm / D
  • 144 height differences 50 µm
  • Comment
  • sigma a posteriori 0.628621 (distance 0.859524,
    horizontal angle 0.450801, vertical angle
    0.563869, height difference 0.782653)
  • Weighted datum

16
Network 2
  • Purpose Check the new floor stability before the
    alignment of the support plates.
  • Description
  • 152 points
  • 121 ring monuments
  • 31 SSRL and BTS monuments
  • 47 laser tracker stations
  • 676 triplet observations
  • Distances 30 µm
  • Horizontal angles 40 µm / D
  • Vertical angles 50 µm / D
  • 123 height differences 50 µm
  • Comment
  • sigma a posteriori 0.825995 (distance 0.832926,
    horizontal angle 0.900147, vertical angle
    0.671085, height difference 0.967139)
  • Free datum

17
Network 3
  • Purpose Assign new values to the SPEAR3
    monuments before fine tuning all necessary
    magnets and vacuum chambers.
  • Description
  • 368 points
  • 122 ring monuments 38 floor, 33 aisle, 50 wall
    and 1 ceiling
  • 45 SSRL monuments
  • 201 magnet TB
  • 40 laser tracker stations
  • 636 triplet observations
  • Distances 40 µm
  • Horizontal angles 40 µm / D
  • Vertical angles 50 µm / D
  • 303 height differences 60 µm
  • Comment
  • sigma a posteriori 1.046304 (distance 0.891794,
    horizontal angle 0.802313, vertical angle
    1.206194, height difference 1.245124)
  • Mixed datum with further 3-parameter
    transformation

18
Datum Controlling Points
HRLN025
19
First Conclusion
  • December 11, 2003 first complete turn of an
    injected electron bunch around the ring.
  • By December 15, 2003 the RF system was
    operational and SPEAR 3 started accumulating beam
    up to 2 mA.
  • January 22, 2004 the stored current reached 100
    mA (maximum current allowed for operation this
    year).
  • March 8, 2004 BL 9 was opened with first users
    March 15.
  • By end of March 2004 BL 10, BL 11, BL 6 and BL 5
    were opened and ready for users.

Extract from the SPEAR 3 Upgrade Project
Close-out Report from April 2004 Measurements
of beam line parameters indicated that the SPEAR
3 optical performance goals were achieved.
20
2004 Network
  • Purpose Map the whole ring as part as the 2004
    Summer/Fall downtime.
  • Description
  • 950 points
  • 143 monuments 37 floor, 32 aisle, 45 wall, 1
    ceiling, 11 others and 17 SSRL points used for
    height only.
  • 807 magnet TBs
  • 44 laser tracker stations
  • 1809 triplet observations
  • Distances 40 µm
  • Horizontal angles 50 µm / D
  • Vertical angles 50 µm / D
  • 270 height differences 50 µm
  • Comment
  • sigma a posteriori 0.938286 (distance 1.287779,
    horizontal angle 0.825724, vertical angle
    0.589023, height difference 0.996919)
  • Mixed datum, offset between the 2 trackers

21
Floor Monuments ChangesNovember 2003 October
2004
22
Floor Monuments ChangesJuly 2003- November 2003
23
Network Weak Spot
BL11 ID
24
Magnet X as-built
25
Magnet Y as-built
26
Final Conclusion
Next beam to beamlines will be Monday, October
18, at 600AM
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