jt: 1 the berkeley lab star tpc distortions in the transverse plane: an update jim thomas

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JT: 1 The Berkeley Lab STAR TPC Distortions in the Transverse Plane: An Update Jim Thomas

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JT: 1The Berkeley Lab

STAR

TPC Distortions in the Transverse Plane:

An Update

Jim Thomas

JT: 2The Berkeley Lab

STARA Mnemonic for Listing the Potential Distortions

ZCal

Barrel EM Calorimeter

Endcap Calorimeter

Magnet

Coils

TPC Endcap & MWPC

ZCal

FTPCs

Vertex Position Detectors

Central Trigger Barrel or TOF

Time Projection Chamber

Silicon Vertex Tracker

RICH

Central Membrane Endwheel and PadplaneOuter Field Cage

Inner Field Cage

JT: 3The Berkeley Lab

STARThe List of Distortions in the Transverse Plane

The list can be enumerated by surfaces:

• Outer field cage corrections • Inner field cage corrections• Central membrane corrections• End-wheel and pad-plane corrections • Pad Row 13 corrections and other local electrostatic defects • Rotation and miss-alignment of sectors with respect to their ideal locations• Rotation of either TPC end-wheel with respect to its ideal location

and by volume:

• Space Charge corrections due to charge in the volume of the TPC • Magnetic field corrections due to B fields in the volume of the TPC• Twist of the TPC with respect to the magnetic field axis and/or the measured map• General coordinate transformations

A few additional items are listed for completeness. (These items affect the drift of the electrons in the Z direction but do not strongly affect the distortions in the transverse plane.)

• Gas composition and variations in the drift velocity• Barometric pressure changes and variations in the drift velocity• Pressure variations as a function of height in the TPC• Temperature gradients in the TPC

JT: 4The Berkeley Lab

STARWe think of our events like this …

Data Taken June 25, 2000.

JT: 5The Berkeley Lab

STARMost of our events look more like this …

JT: 6The Berkeley Lab

STARSpaceCharge from (all) events cause distortion

Z / 5 cm

Rad

ius

/ 5 c

m

Z

Radius

Dis

tort

ion

JT: 7The Berkeley Lab

STARModel for the distortions

• Old Model– Beam gas events leave a uniform deposition of

charge in the TPC

– The charge from the collisions is not significant

• New Model– Beam gas events leave a 1/R2 distribution of

charge in the TPC

– The charge from the collisions is not significant in the 2001 data, but will be in the future (?)

JT: 8The Berkeley Lab

STARUniform .vs. 1/R2 Space Charge Distribution

RadialDistortions

Z Z

Radius

RadiusD

isto

rtio

n

Dis

tort

ion

JT: 9The Berkeley Lab

STARTwo sources of SpaceCharge

• Beam gas and other up stream events– not synchronous with our trigger

– Scales with beam intensity (not Luminosity)

– 1/R2 distribution of charge (?)

• The collisions at STAR– synchronous with our trigger

– Scales with Luminosity

– A/R + B/R2 distribution of charge (?)

• In the future, the average Luminosity will go up a factor of 40 but the beam intensity will only go up a factor of 2 to 4

– We have to prepare for a significant increase in space charge due to the collisions in the detector.

We have to be able to distinguish the two sources of distortion

JT: 10The Berkeley Lab

STARA Wide Range of Charge Distributions

1/R3 1/R2 Wieman’s HiJet

1/R Linear 2:1 Linear

These (and other) Distributions are Available in StMagUtilities

Radius

Vo

ltag

e

JT: 11The Berkeley Lab

STAR2 Equations, 2 Unknowns

• We can simultaneously fit the DCAs and match the steering at the RICH due to the beam gas induced space charge

– Choose the right charge distribution 1/R, 1/R2, HiJet, etc.

– Choose the RICH scaler normalization constant

Variations in Charge Shape

-1500.0

-1000.0

-500.0

0.0

500.0

1000.0

1500.0

1 3 4 51/

R 6 10 16

Wiem

an

1/R**2

1/R**3

Shape Parameter

Dis

pla

cem

ent

at R

ICH

in

mic

ron

s

delta Rich

with the DCA held constant

JT: 12The Berkeley Lab

STARThese Items on the List Are Ready to Go

The list can be enumerated by surfaces:

Outer field cage corrections Inner field cage corrections• Central membrane corrections• End-wheel and pad-plane corrections Pad Row 13 corrections and other local electrostatic defects Rotation and miss-alignment of sectors with respect to their ideal locations Rotation of either TPC end-wheel with respect to its ideal location

and by volume:

Space Charge corrections due to charge in the volume of the TPC Magnetic field corrections due to B fields in the volume of the TPC Twist of the TPC with respect to the magnetic field axis and/or the measured map General coordinate transformations

A few additional items are listed for completeness. (And these I don’t know about.)

• Gas composition and variations in the drift velocity• Barometric pressure changes and variations in the drift velocity• Pressure variations as a function of height in the TPC• Temperature gradients in the TPC

JT: 13The Berkeley Lab

STARConclusions

• Tools are available to calculate all known distortions – in the transverse plane

– gain, t0, and drift velocity corrections have not been discussed

• SpaceCharge corrections are significant – especially at 40x <L>

• We need to track the beam current and/or the distribution of charge in the TPC for untriggered events. We will need scalers and diagnostics for each source of charge

– Monitor L– Monitor beam current

• The RICH Mult Scaler is gone and we need a replacement

• Recent progress with the laser cluster finder means we might be able to use this data …

JT: 14The Berkeley Lab

STARDCA, Steering at the RICH, and p

• The RICH Scaler has an arbitrary normilization

• The DCA’s have been tuned to be the same in both cases

• p is different by a factor of 2

• Steering at the Rich changes sign under these conditions

Uniform Charge Distribution (0.004)

-2500.0

-2000.0

-1500.0

-1000.0

-500.0

0.0

500.0

0 50 100 150 200 250

Z axis

Dis

pla

cem

ent

(mic

ron

s o

r M

eV)

DCA

delta Rich

delta p (x10)

Event Charge Distribution (0.0021)

-2500.0

-2000.0

-1500.0

-1000.0

-500.0

0.0

500.0

1000.0

0 50 100 150 200 250

Z axis

Dis

pla

cem

ent

(mic

ron

s o

r M

eV)

DCA

delta Rich

delta p (x10)