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Møller Polarimeter Status Update 1. Møller hardware status (detectors and targets) 2. Systematics for SANE 3. Plan Dave Gaskell SANE Collaboration Meeting May 30, 2008

Møller Polarimeter Status Update

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Møller Polarimeter Status Update. Møller hardware status (detectors and targets) Systematics for SANE Plan Dave Gaskell SANE Collaboration Meeting May 30, 2008. Hall C Møller Polarimeter. Superconducting solenoid  Brute force out of plane magnetization. Scintillators  set “tune” - PowerPoint PPT Presentation

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Page 1: Møller Polarimeter Status Update

Møller Polarimeter Status Update

1. Møller hardware status (detectors and targets)

2. Systematics for SANE

3. Plan

Dave Gaskell

SANE Collaboration Meeting

May 30, 2008

Page 2: Møller Polarimeter Status Update

Hall C Møller Polarimeter

Superconducting solenoid Brute force out of plane magnetization

Scintillators set “tune”Calorimeter measurement

Page 3: Møller Polarimeter Status Update

Detectors

One dead scintillator on left arm appeared during GEp

Scintillators refurbished before G0 Back angle Additional repairs before GEp

Page 4: Møller Polarimeter Status Update

Targets

Present target configuration optimized for “high current” running 1-2 A

At 100 nA, dP/P=1% (stats) would take 2.4 hours on 4 m target (5.9 GeV)

SANEReplace 1 m foil with 10 m foilReplace “not accessible” with 20 m foil and make accessible with new actuator

Kicker test target

4 m foil

1 m foil

Not accessible

GEp Configuration

Page 5: Møller Polarimeter Status Update

Systematics: G0 Forward AngleSource Uncertainty dAsy./Asy. (%)

Beam position x 0.5 mm 0.15

Beam position y 0.5 mm 0.03

Beam direction x 0.15 mr 0.04

Beam direction y 0.15 mr 0.04

Q1 current 2% 0.10

Q2 current 1% 0.07

Q2 position 1 mm 0.02

Multiple Scattering 10% 0.12

Levchuk effect 10% 0.30

Collimator positions 0.5 mm 0.06

Target temperature 50% 0.05

B-field direction 2o 0.06 0.37

B-field strength 5% 0.03

Spin polarization in Fe 0.25

Leakage 30 nA 0.2

High current extrap. 1%/40 uA 1.0

Solenoid focusing 100% 0.1

Elec. DT. 100% 0.04

Charge measurment 0.02

Monte Carlo Statistics 0.28

Unknown accelerator changes 0.5

Total 1.32

Systematic error budget from G0 Forward Angle expt.

dP/P = 1.32%

Page 6: Møller Polarimeter Status Update

Systematics: SANESource Uncertainty dAsy./Asy. (%)

Beam position x 0.5 mm 0.15

Beam position y 0.5 mm 0.03

Beam direction x 0.15 mr 0.04

Beam direction y 0.15 mr 0.04

Q1 current 2% 0.10

Q2 current 1% 0.07

Q2 position 1 mm 0.02

Multiple Scattering 10% 0.12

Levchuk effect 10% 0.30

Collimator positions 0.5 mm 0.06

Target temperature 50% 0.05

B-field direction 2o 0.06 0.37

B-field strength 5% 0.03

Spin polarization in Fe 0.25

Leakage 30 nA 0.2

High current extrap. 1%/40 uA 1.0

Solenoid focusing 100% 0.1

Elec. DT. 100% 0.04

Charge measurment 0.02

Monte Carlo Statistics 0.28

Unknown accelerator changes 0.5

Total 1.32

1. No “high current extrapolation” 2. Leakage more important

dP/P < 1.5%?

Page 7: Møller Polarimeter Status Update

Systematics: SANE

It is unlikely Wien will be set for maximum polarization to Hall C during SANE

At 5 pass and high energy (5.9 GeV) small changes in the beam energy can impact the polarization in the Hall

Example: Wien set for 80% of maximum in Hall C at 5.9 GeV

1 MeV shift in beam energy gives 2.3% change in polarization in Hall

OptimumSANE?

Page 8: Møller Polarimeter Status Update

Hall C Møller during GEp

Some hint of dependence of polarization on QE!

Page 9: Møller Polarimeter Status Update

Collimator Issues

General philosophy:Let collimators in front of detectors determine acceptance

Collimators between Q1 and Q2 “clean up” backgrounds do not impact acceptance

Page 10: Møller Polarimeter Status Update

Collimator Issues

At 5.9 GeV, collimators between Q1/Q2 come close to impinging on acceptance

Collimators 6&7 can collide – may cause reproducibility problems

Page 11: Møller Polarimeter Status Update

Møller Measurement Plan

Measurements desired every 2-3 days

Two options:1. RSS-style general procedure that anyone on shift

can follow Can make measurements anytime – whenever

convenient Results may be a little less reliable

2. G0 Forward-style: “small” group makes all measurements (“small”= at least 5-6 people) Measurements need to be scheduled More reliable polarization measurements smaller systematic errors