Measurements as a Tool to Monitor Magnet Production

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Measurements as a Tool to Monitor Magnet Production Animesh Jain Brookhaven National Laboratory Upton, New York 11973-5000, USA US Particle Accelerator School on Superconducting Accelerator Magnets Phoenix, Arizona, January 16-20, 2006

Transcript of Measurements as a Tool to Monitor Magnet Production

Measurements as a Toolto Monitor

Magnet Production

Animesh JainBrookhaven National Laboratory

Upton, New York 11973-5000, USA

US Particle Accelerator School on Superconducting Accelerator Magnets

Phoenix, Arizona, January 16-20, 2006

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL1

Introduction• The primary goal of magnetic measurements is to

provide the data necessary for smooth operation of accelerators, or for accurate analysis of data from detectors. (Need based measurements)

• Field quality is very sensitive to small changes in conductor placement and material properties. This makes magnetic measurements an excellent tool to monitor magnet production.

• Warm measurements, carried out in the early stages of production, can be particularly beneficial in providing a timely feedback.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL2

Examples• Nearly all large scale magnet productions have

several instances where magnetic measurements have indicated a problem with the production.

• The problems could vary over a wide range, e.g.– Parts that are slightly out of tolerance– Material with undesirable magnetic properties– Incorrect or missing parts– Electrical shorts

• With a timely feedback, one can prevent use of defective magnets in complex assemblies, or minimize affected magnets in a large production.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL3

Role of Data Analysis• Some problems cause a drastic change in field

quality, and are hard to miss.

• Some problems may be more subtle (e.g. a slow trend in the dimension of parts) and may require attention to detail.

• Some localized problems in a long magnet, even if drastic, may not show up in the integral field quality. Local variations must be studied.

• In all cases, once a problem is confirmed, it is important to provide useful clues as to what may possibly be wrong. This is not always easy.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL4

Dipole Example from RHICDipole No. 149 (DRG189): Axial scan with 1 m long mole in 1 m steps

0.7028

0.703

0.7032

0.7034

0.7036

0.7038

0.704

0.7042

0.7044

0 1 2 3 4 5 6 7 8Axial Position (m)

Tra

nsfe

r F

unct

ion

(T/k

A)

Warm meas. at the vendor’s site showed an unusual drop in transfer function (0.18%) at one location.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL5

Dipole No. 149 (DRG189): Axial scan with 1 m long mole in 1 m steps

-2.0

-1.6

-1.2

-0.8

-0.4

0.0

0.4

0.8

1.2

1.6

2.0

0 1 2 3 4 5 6 7 8Axial Position (m)

Nor

mal

Qua

drup

ole

(uni

t at

25

mm

)

-16.0

-14.0

-12.0

-10.0

-8.0

-6.0

-4.0

-2.0

0.0

0 1 2 3 4 5 6 7 8Axial Position (m)

Skew

Qua

drup

ole

(uni

t at

25

mm

)

Dipole Example from RHIC

Normal quadrupole term was OK

Large –veChange in Skew quad

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-5.0

-4.0

-3.0

-2.0

-1.0

0.0

1.0

2.0

3.0

0 1 2 3 4 5 6 7 8Axial Position (m)

Nor

mal

Sex

tupo

le (

unit

at

25 m

m)

-1.0

-0.8

-0.6

-0.4

-0.2

0.0

0.2

0.4

0.6

0.8

1.0

0 1 2 3 4 5 6 7 8Axial Position (m)

Skew

Sex

tupo

le (

unit

at

25 m

m)

Dipole No. 149 (DRG189): Axial scan with 1 m long mole in 1 m steps

Dipole Example from RHIC

Skew Sextupoleterm was OK

Large –vechange in Normal Sextupole

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL7

-0.4-0.20.00.20.40.60.81.01.21.41.61.82.02.2

0 1 2 3 4 5 6 7 8Axial Position (m)

Skew

Oct

upol

e (u

nit

at 2

5 m

m)

0.9

1.0

1.1

1.2

1.3

1.4

1.5

1.6

1.7

1.8

1.9

2.0

0 1 2 3 4 5 6 7 8Axial Position (m)

Nor

mal

Dec

apol

e (u

nit

at 2

5 m

m)

Dipole No. 149 (DRG189): Axial scan with 1 m long mole in 1 m steps

Dipole Example from RHIC

Large +vechange in Normal Decapole

Large +vechange in Skew Octupole

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL8

Dipole Example from RHIC• The unusual changes in transfer function, and

several harmonics, indicated a definite problem with the construction of the magnet.

• Only even skew and odd normal harmonics were affected. Even normal and odd skew terms were unaffected.

• Left-right anti-symmetry was preserved, buttop-bottom symmetry was not preserved.

• Changes in the signs of harmonics indicated that the problem is closer to the pole, than midplane.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL9

0.7024

0.7026

0.7028

0.7030

0.7032

0.7034

0.7036

0.7038

0.7040

0.7042

6 6.5 7 7.5 8 8.5Axial Position (m)

Tra

nsfe

r F

unct

ion

(T/k

A)

-24.0-22.0-20.0-18.0-16.0-14.0-12.0-10.0-8.0-6.0-4.0-2.00.02.0

6 6.5 7 7.5 8 8.5Axial Position (m)

Skew

Qua

drup

ole

(uni

t at

25

mm

)

Dipole No. 149 (DRG189): Scan with 1 m long mole in 0.15 m stepsDipole Example from RHIC

A finer scan indicated TWO similar defects !

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL10

-8

-7

-6

-5

-4

-3

-2

-1

0

1

2

6 6.5 7 7.5 8 8.5Axial Position (m)

Nor

mal

Sex

tupo

le (

unit

at

25 m

m)

-0.5

0.0

0.5

1.0

1.5

2.0

2.5

3.0

6 6.5 7 7.5 8 8.5Axial Position (m)

Skew

Oct

upol

e (u

nit

at 2

5 m

m)

Dipole No. 149 (DRG189): Scan with 1 m long mole in 0.15 m stepsDipole Example from RHIC

Only one of the defects covered by the mole

BOTH defects covered by the mole

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL11

Dipole Example: Summary• The nature of harmonics indicated that the coil

turns near the upper pole have moved symmetrically towards the vertical axis.

• There were two defect regions, each about 0.15m long.

• RHIC dipoles use 0.15 m long RX630 pole spacers between coil and yoke. The end section spacers are different from the straight section.

• The end type of spacers were inadvertently used in the straight section. This was verified later.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL12

Shorts in a Multilayer Magnet• BNL has recently built several multilayer

magnets for the HERA upgrade program at DESY, Hamburg.

• These magnets were fabricated by winding a 1 mm diameter superconducting cable using an automatic winding machine.

• The magnets had several layers of coils with different multipolarities.

• On two occasions, the coil curing process produced electrical shorts.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL13

Splice Between “Sub-coils”

Splice

Pole Lead

Pole Lead

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Electrical Short in QH0103• Large changes in the harmonics were observed in the

main quadrupole of the magnet QH0103 after all the layers were completed.

• Magnetic measurements were NOT carried out after each step. So, it was difficult to judge at what step the problem could have occurred.

• Warm measurements were carried out at 0.25A on individual layers using the voltage taps as current leads.

• The measurements indicated a problem with the 2nd quad layer, which was burried under 3 more layers.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL15

Harmonic Changes in QH0103: Q2as wound final meas. Change

T.F.(T/m/kA) 8.6534 8.6956 0.49%b3 -2.91 16.47 19.37b4 0.77 1.39 0.62b5 -0.50 -7.82 -7.32b6 -0.98 5.66 6.64b7 -0.19 -2.81 -2.62a3 -1.82 16.71 18.52a4 -4.12 -21.69 -17.57a5 -0.12 7.77 7.89a7 -0.16 -2.64 -2.47

Selected harmonics in “units”at 31 mm reference radius

⇐ increase was asexpected

b3 = normal sextupole, and so on.

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL16

Determining the Problem Quadrant

+ =

Normal Quad +ve Normal Sextupole

+ =

Missing Current in the 2nd Quadrant

Weaker field on LEFT

S

S N

NS S

N

N N

S

Normal Quad

S

S N

N

+ve Skew Sextupole

S

S

N

N

NS

Weaker field on TOP

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL17

Modeling Field Errors in QH0103• Most likely area: pole lead in the 2nd quadrant.

• Would bypass current from the pole-most turn.

-6.5

0

6.5

-6.5 0 6.5X (cm)

Y (c

m)

Zero Current

QH0103: Q2

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL18

Computed Vs Measured Changes

-60

-50

-40

-30

-20

-10

0

10

20

30

40

50

60

2 3 4 5 6 7 8 9 10 11 12 13 14 15 16Harmonic Number

Cha

nge

in H

arm

onic

(un

its

at 5

0 m

m)

Normal: MeasuredNormal: CalculatedSkew: MeasuredSkew: Calculated

Note: Reference radius increased from 31 mm to 50 mm to clearly show the higher harmonics

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL19

QH0103: Q1, Q2, Q3 Layers

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL20

QH0103: Repair of Q2 ShortFortunately, it was possible to carefully cut into the S-glass wrap to reach the pole lead of Q2, without affecting other layers. Thus, a repair could be performed without sacrificing any layer.

2 turns of Q2 exposed for repair

Q3 LeadsQ3 Leads

Q1 LeadsQ1 Leads

USPAS, Phoenix, January 16-20, 2006 Animesh Jain, BNL21

Conclusions• Warm measurements have proved to be a very

sensitive tool to monitor magnet production.• Accurate harmonic information, coupled with

a model analysis, can provide exact location of defects. This may allow for efficient repairs in some cases.

• Gross errors are often easy to detect and model. Subtle changes may be hard to model.

• One must be careful in interpreting data from long probes. A “deconvolution” of data may be needed to better characterize the defects.