NuStorm Implementation at Fermilab
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Transcript of NuStorm Implementation at Fermilab
3/27/20131
NuStorm Implementation at Fermilab
Michael GeelhoedFermilab AD/EBD
Photo by Marty Murphy
Michael Geelhoed Fermilab AD EBD3/27/20132
• Location• Primary Beamline• Main Injector Specifics• Components • Cost• Safety Considerations
Focus on Fermilab specific aspects
Topics covered yesterday:
Target ModulePion CaptureSpecial Magnet Design
Decay RingFar DetectorNear Detector
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Location of Facility
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Location of Facility
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Location of Facility
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Main Injector Absorber Area
Location of Facility
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-20 80 180 280 380 480 580 680 780 8800
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XBEAM (1 sigma)YBEAM (1 sigma)XBEAM (95%)YBEAM (95%)Aper XAper Y
Stationing (ft)
Half
Wid
th (m
m)
NuStorm Primary Beamline
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-10 90 190 290 390 490 590 690 790 890
-300
-200
-100
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ALPHAXALPHAY
Stationing (ft)
-10 90 190 290 390 490 590 690 790 8900
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BETAXBETAY
Beta
(m)
NuStorm Primary Beamline
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-2 -1.5 -1 -0.5 0 0.5 1 1.5 2
-0.25
-0.2
-0.15
-0.1
-0.05
0
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0.1
0.15
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Y 1 SigmaX 1 Sigma
X and Y (mm)
X’ a
nd Y
’ (m
r)
-2 -1.5 -1 -0.5 0 0.5 1 1.5 2
-0.25
-0.2
-0.15
-0.1
-0.05
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0.05
0.1
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Y 6 sigmaX 6 sigma
X and Y (mm)
X’ a
nd Y
’ (m
r)
Beam on Target
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0 50 100 150 200 250 300 350 400 450 5000
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XBEAM (95%)YBEAM (95%)Aper XAper Y
Half
Wid
th (m
m)
0 50 100 150 200 250 300 350 400 450 5000
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XBEAM (95%)YBEAM (95%)Aper XAper Y
Stationing (ft)
Half
wid
th (m
m)
Q001 Q002 Q003 Bermpipe
MI Abort line Reconfiguration
Michael Geelhoed Fermilab AD EBD 113/27/2013
Move Q002 and Q003 upstream by 30’ and 23’, along with different currents, NS/Abort beam reduces in size through the bermpipe
Current (Amps) Present Future
Q001 2770.5 1883.2
Q002 2828.0 1423.9
Q003 2770.5 853.0
MI Abort line Reconfiguration
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Find a suitable proton beam(Energy, pulse length, structure, etc.)
Beam Parameters:
120 Gev/c protons*1.33 second cycle time**1.57 µs pulse length per “batch”7.0E12 protons per pulse100 kW Beam Power
Available “Now”
Shielded for 400 kW
* Primary Beamline can be converted to 60 Gev/c ** Post 2013 Shutdown
Possible MI Capabilities
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Cost Quantity Cost ($M)
Dipoles 11 1.10
Quads 5 1.30
Trims 18 0.26
BPMs 12 0.08
Multiwires 11 0.22
Toroids 3 0.06
Enclosure length 432 ft 4.32
Total 7.34
Total x 3.2 (Contingency + Escalation) 23.50
Estimates provided by Fermilab Technical Division Project CoordinatorEstimates given by Fermilab AD/Instrumentation Dept. for LBNE Estimates provided by Fermilab’s FESS EngineeringEstimate based on Project X Management data
Beamline Components
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Magnet Images
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Magnet costs
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Escalated values
Magnet style Series Date Escalation Labor ea Materials ea Total ea Qty Extended Total Comment
B2 Dipole BDM 2008 1.0958 $ 102,523 $ 11,287 $ 113,810 9 $ 1,024,288 Est for LBNE Job 440: Burn, clean-
up, reconstruct
3Q-120 QQQ 2009 1.0711 $ 90,958 $ 170,313 $ 261,271 5 $ 1,306,356 Est for LBNE Job 465 Build new
EDB EDBC 2012 1 $ 5,200 $ 2,700 $ 7,900 2 $ 15,800
Recently rebuilt with PEEK and 4 lg power flags (assumes existing
magnet)
IDH IDH 2004 1.2112 $ 10,780 $ 4,481 $ 15,261 8 $ 122,089 (23) were built in 2004 Job 188
IDV IDV 2004 1.2112 $ 10,780 $ 5,490 $ 16,270 8 $ 130,160 (same as IDH but 22.5% larger
M&S)
$ 2,598,694 * Estimates provided by TJ Gardner TD Project Coordinator
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Safety Consideration
Critical Devices include: NSHV1- Single EDB magnet bends beam away from MI Absorber to NS notch NU1H1- 5 B2 magnet string in NU1
Consideration taken: 50’ away from MI beamline center offers protection for construction installation and access
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Safety Beamline Map
3/27/2013
MARS15 simulation run for Critical Device Justification N.V. Mokhov, "The MARS Code System User's Guide", Fermilab-FN-628 (1995); N.V. Mokhov, O.E. Krivosheev, "MARS Code Status", Proc. Monte Carlo 2000 Conf., p. 943, Lisbon, October 23-26, 2000; Fermilab-Conf-00/181 (2000); N.V. Mokhov, "Status of MARS Code", Fermilab-Conf-03/053 (2003); N.V. Mokhov, K.K. Gudima, C.C. James et al, "Recent Enhancements to the MARS15 Code", Fermilab-Conf-04/053 (2004); http://www-ap.fnal.gov/MARS/. MARS was developed in part with Government funding provided under DOE Contract DE - AC02 -76CH03000.
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Thank You
Special thanks to:Steve Dixon
Tommy LackowskiRonald Jedziniak
TJ GardnerDallas Heikkinen
Robert Riley
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Backup Slides
3/27/2013
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Backup Slides
3/27/2013