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Single Aperture Orbit Corrector: Progress on MCBXFB design WP3 Meeting J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

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Page 1: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Single Aperture Orbit Corrector:

Progress on MCBXFB design

WP3 Meeting

J. García, F. Toral (CIEMAT)

P. Fessia (CERN)

January, 26th 2015

Page 2: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Requirements & specifications. Latest design presented. Mechanical analysis of the iron ring magnetic

design. New magnetic optimization. Conclusions & decisions to be made. Next steps.

Index

2

Page 3: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Requirements & specifications

3

Page 4: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

MCBXFB Requirements

4

Magnet configuration Combined dipole (Operation in X-Y square)

Minimum free aperture 150 mm

Integrated field 2.5 Tm

Baseline field for each dipole 2.1 T

Magnetic length 1.2 m

Physical length 1.505 m

Working temperature 1.9 K

Nominal current < 2500 A

Field quality < 10 units (1e-4) *

Fringe field 40 mT *

Iron geometry MQXF iron holes

Strand parameters

Cu:Sc 1.75Strand diameter 0.48 mm

Metal section 0.181 mm2

Nº of filaments 2300Filament diam. 6.0 µm

I(5T,4.2K) 200-210 AJc 2800-3300 A/mm2

Cable parameters

No of strands 18Metal area 3.257 mm2

Cable thickness 0.845 mmCable width 4.370 mmCable area 3.692 mm2

Metal fraction 0.882Key-stone angle 0.67 degInner Thickness 0.819 mm

Outer Thickness

0.870 mm

Strand & cable specificationsInsulation: Fibre glass sleeve• This method provides stiffer coils for an

easier double layer winding.• Need validation test of a suitable binder:

• Ceramic binder is not applicable (only in cured state).

• Some PVA studies are ongoing but compatibility with impregnation has to be demonstrated.

• Ceramic binder substitute (suggestion by CTD) is being tested by CERN.

*To be discussed at this meeting

Page 5: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Latest design presented(November 2014)

5

Page 6: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

6

Two main problems:

Saturation at nominal current for both dipoles causes the increasing of sextupoles:◦ ∆b3= 37 units◦ ∆a3= -25 units.

Large radial deformations (causing possible poor training).

Two solutions proposed:

New magnetic design using an iron ring placed further away.

Larger collars in order to increase the stiffness of the assembly and make them self-supporting.

Worst case:IID & IOD variation from 10% to 100%

Page 7: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

7

Current increase from previous design: IID=1885 A (prev. 1560 A) IOD=1870 A (prev. 1340 A) Greater forces!Saturation multipoles: b3= 17 (prev. 37) a3= 18 (prev. 24)

New magnetic design

Ansyssimulationusing the

new forces(108% IN)

Worst case:IID=100% IOD= Var. from 10% to100%

Page 8: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Mechanical analysis of theiron ring magnetic design

8

Page 9: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

9

Any of the actions taken to increase the stiffness of the assembly decreased the radial displacements of the outer coils.

Ellipticity

Page 10: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

10

However, the action of an external shell or increasing the outer collars thickness do not reach the inner coils, given the assembly gap between inner collars and outer coils.

GAP

GAP

Outerpressure

Magnetic forces (Both dipoles at

108% IN)

The only way to decrease the inner dipole ellipticity is to increase inner collars thickness.

Page 11: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

11

New geometry

OD Max Ellipticity= 0.3175 mm(prev 0.3485 mm)ID Max Ellipticity= 0.3064 mm(prev 0.4828 mm)

Geometrical changes:• Inner collar thickness increased

in 6 mm (21 mm -> 27 mm).• Outer collar thickness increased

in 2 mm (31 mm -> 33 mm).• Outer dipole aperture increased

from 218 mm to 230 mm.• Outer collar diameter increased

from 300 mm to 316 mm.

• It is difficult to put a limit on the radial displacements. • The main goal has been to make it as stiff as

possible while keeping reasonable dimensions.• It has to be highlighted also that each mm of

additional steel has less effect than the previous one.

Page 12: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

12

Mechanical analysis: Contact between coils and collars

1

2

21

1 2

Page 13: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

13

Mechanical analysis: Coil stress

Assembly Cooldown Load

All these results were obtained using the inner Titanium tube.Possible re-evaluation considered.

100% IN

Low radial tension at spacers edges, caused by friction

Low azimuthal tension caused

by friction

Page 14: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

New magnetic optimization

14

Page 15: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Inner coil (ID) & Outer Coil (OD) parameters

Units Whole iron Iron ring Only cryostat

Nominal field 100% (ID) T 2.11 2.11 2.11

Nominal field 100% (OD) T 2.11 2.11 2.11

Nominal Field (Modulus, 100% ID & 100% OD) T 2.99 2.99 2.99

Nominal current (ID) A 1590 1870 1950

Nominal current (OD) A 1390 1895 2070

Coil peak field (Modulus, 100% ID & 100% OD) T 3.94 (ID) 4.18 (ID) 4.25 (ID)

Working point (Modulus, 100% ID & 100% OD) % 48.49 53.39 54.8

Max fringe field, 20 mm out of the cryostat (Modulus, 100% ID + 100% OD)

mT 29 100 165

Sextupoles variation ∆b3 / ∆a3 (Worst case) units 37 / -21 15 / 14 2 / 5

Iron yoke Inner Diam. mm 316 432 -

Iron yoke Outer Diam. mm 610 610 -

Torque 105 Nm/m 1.2 1.42 1.48

Mean stress at the coil and collar nose interface

MPa 84 98 102

15

Using the new geometry:• Outer dipole aperture = 230 mm.

• Collars outer diameter = 316 mm.

Page 16: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

16

Sextupoles monitoring

Page 17: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

17

Field quality optimization difficulties

o Other iron geometries were tested, with similar or worse field quality results:

o The difficulty comes because the field changes in two ways depending on the powering scenario: Orientation and intensity.

o One of these variations could be assumed optimizing the iron geometry.

o Both of them combined make any optimized geometry useless when the powering scenario changes, because symmetry conditions are lost.

Page 18: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

18

Fringe field and iron screening effectiveness

o It is not possible to screen the field below 40 mT without the whole iron, a lot of magnetic material would be necessary.

o Adding a warm screen and measuring the fringe field 20 mm from its surface:• Rin= 467 mm, Thickness = 10mm, Max Fringe field = 131 mT.• Rin= 467 mm, Thickness = 50mm, Max Fringe field = 31 mT.

o Other magnetic materials like mumetal would not be a solution, since they have higher permeability, but lower saturation field.

o The main problem is that we deal with a dipole: the dipole field decays as 1/r2

compared to quadrupole field which decays as 1/r3.

o Therefore, we should choose between:• Higher fringe field or• Higher variation of the multipoles with the current (when magnetic

materials shield the dipole field).

Page 19: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

19

Coil ends: First results (without iron)

o Field quality achieved but peak field still high. o Several approaches being evaluated. Currently

checking how splitting blocks could help.o Coil ends length 200 mm.≅o Coils length 1400 mm.≅o Total magnet length = 1505 mm (Current layout).

Page 20: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Conclusions & decisions to be made

20

Page 21: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Conclusions

21

Mechanical design:◦ Whichever the mechanical design used, the radial

displacements in the inner dipole can only be contained using the inner collar.

◦ The thickness of the inner collar will depend on the current in the inner coil and the radial displacement allowed for the inner coil.

Magnetic design:◦ It is not achievable to meet both fringe field and field

quality requirements simultaneously.

Page 22: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Decisions to be made

22

Inner & Outer dipole apertures.

Iron geometry (if any).

Page 23: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Next steps

23

February ‘15: 3D Magnetic Optimization

March ’15: Winding Machine.

April ‘15: Short mechanical model.

October ‘15: First coil.

CERN: Binder tests.

Page 24: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Thanks for your attention

24

Page 25: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Annexes

25

Page 26: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Mechanical design: Challenges to face

26

As a combined dipole that requires a square range of operation in X and Y axis, a large torque arises when both coils are powered.

Due to the expected radiation dose a solution based on mechanical clamping is required to mechanically fix the coils and guarantee the magnet performance.

Other major challenges:

Mechanical model◦ Powered with 108% of nominal current for sizing purposes.◦ Material properties used:

Material E [Gpa] u [-] CTE [K-1]

Coils & spacers (Impregnated) NbTi+Cu 40 0,0032 1.1*10-5

Collars StainlessSteel 193293K/2104.3K 0,0028 0.983*10-5

Inner tube Ti 130 0,0017 0.603*10-5

Radial inward forces at the inner dipole Inner titanium tube

Large azimuthal displacements of the coils Azimuthal interference at collar noses

Large radial deformations of the assembly Large self-supporting collars

Challenge Solution proposed

Page 27: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Considerations on a MCBXFB design based on a canted cosine-theta coil configuration

27

Comparing the main challenges in the case of MCBXFB design for both designs:◦ The torque between nested dipoles:

It will be the same for both designs.◦ The separation of the pole turn from the collar nose due to the Lorentz forces:

It does not happen in the CCT dipole (azimuthal forces support). In the pure cosine-theta it can be overcome with a small interference between the collar

nose and the pole turn of the coil.◦ The elliptical deformation of the support structure under Lorentz forces:

In a CCT dipole the outer formers should hold the outwards radial forces coming from the inner layers, which complicates significantly the assembly and fabrication.

The assembly of two nested collared coils is not easy, but seems more affordable.

The CCT configuration has not been broadly used up to now, so other open questions are:◦ The handling of the axial repulsive forces between layers.◦ The influence of the cable positioning accuracy on the field quality.◦ The training of a large and high field superconducting dipole.◦ The protection of the magnet in case of quench.◦ Formers materials to be used (insulation, stiffness and easily machining required).◦ Coils impregnation.

Page 28: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Some useful expressions to understand where mechanical stresses come from

28

𝐼𝑇=∫− 𝜋2

𝜋2

𝐽 dl=∫− 𝜋2

𝜋2

𝐽 0 cos𝜃𝑅 dθ=2 𝐽 0𝑅 𝐽 0=𝐼 𝐼𝐶2𝑅

𝑇𝑙= �⃗�× �⃗�

𝑙=𝐵𝑂𝐶

𝑙 ∫− 𝜋2

𝜋2

𝑆 ∙ 𝐼=𝐵𝑂𝐶 ∫−𝜋2

𝜋2

2𝑅𝐼𝐶 cos𝜃 𝐽 0 cos𝜃 𝑅𝐼𝐶dθ

dl

d=2Rcosθ

IIC-IIC

BOC

J[A/m]=J0cosθ

�⃗�

𝑻𝒍

=𝝅𝟐𝑹𝑰𝑪𝑩𝑶 𝑪 𝑰 𝑰𝑪

T

R

R

h F

F

𝝈𝜽𝒄𝒐𝒏𝒅=𝑭𝑨

=𝑻 /𝟐𝑹𝒍𝒉

=𝑻 /𝒍𝟐𝑹𝒉

𝑻𝒍

=𝝁𝟎𝝅𝟖

𝑰 𝑰𝑪 𝑰𝑶𝑪

𝑹𝑰𝑪

𝑹𝑶 𝑪 (𝑹𝒀𝟐+𝑹𝑶𝑪

𝟐

𝑹𝒀𝟐 )*

* Linear Iron

Page 29: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

29

Model settings and convergence challenges

2D Ansys Workbench model. 0.5-mm-thick shell elements at the collars. 1-mm-thick shell elements for the rest of the assembly.

Load steps. t=0-1: Contact offset (pre-stress). t=1-2: Assembly cooldown. t=2-3: EM forces (exported from Maxwell, 108% Nominal current).

Convergence/stability challenges No symmetry boundary conditions can be used. DOF more

difficult to constrain. Many parts involved and linked by contact. Frictional contacts

showed better performance that frictionless ones. Techniques used to achieve convergence:

Adding extra boundary conditions. Tuning up contact settings at problematic zones (Stabilization

dumping factor, Normal stiffness, ramped effects...).

Page 30: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Materials

30

Cable, wedges and inter-layer insulation: glass fibre sleeve impregnated with binder treatment as hardener (PVA to be studied).

Wedges: machined from ETP copper. End spacers: 3D printed in stainless steel. Ground insulation: Polyimide sheets Vacuum impregnated coils, radiation hard resin (cyanate-ester

blend). Collars: Machined by EDM in stainless steel. Iron: To be evaluated. Connection plate: Hard radiation resistant composite, like Ultem. End plates: Stainless steel. Inner pipe: Titanium grade 2 if grade 5 is not available.

Page 31: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Winding

31

Customized winding machine lent by CERN◦ New beam: 2.5 m long.◦ Electromagnetic brake.◦ Horizontal spool axis.

Winding process◦ Stainless steel mandrel protected with a polyimide sheet.◦ Binder impregnation and curation.◦ Outer layer will be wound on top of the inner one with an

intermediate glassfiber sheet for extra protection.◦ Vacuum impregnation with hard radiation resin.

Page 32: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Assembly

32

Collars placed around the coils with a vertical press (custom tooling required).

Layer of protection between both dipoles, likely a glass fibre sheet

Innermost turn of the coils will be protected by a stainless steel sheet from the collar nose sliding.

Iron laminations around the coil assembly.

Page 33: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

Protection

33

Page 34: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

CIEMAT in-house developed codebased on finite difference method :Optimistic assumptions of the model

34

Rutherford cable is modeled as a monolithic wire with the same metallic area, discarding the voids or internal volumes filled with resin.

The wedges are not modeled. Quench origin is placed at the innermost turn,

although it is not where the peak field is placed when both coils are powered.

A uniform magnetic field is assumed in the wires, equal to the peak field.

Page 35: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

MCBXFB: No damping resistance included

35

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10

200

400

600

800

1000

1200

1400

1600Current decay in quench

Cu

rren

t (A

)

Time (s)0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

0

20

40

60

80

100

120

140

160

180

200Maximum temperature in quench

Tem

per

atu

re (

K)

Time (s)

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10

0.05

0.1

0.15

0.2

0.25

0.3

0.35

0.4Coil resistance in quench

Res

ista

nce

(O

hm

)

Time (s)0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1

0

50

100

150

200

250Quenching coil voltage

Vo

ltag

e (V

)

Time (s)

Preliminary

Page 36: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

MCBXFB: Damping resistance = 0.3 Ω (0.1 s delay)

36

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.90

200

400

600

800

1000

1200

1400

1600Current decay in quench

Cu

rren

t (A

)

Time (s)0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9

10

20

30

40

50

60

70

80

90Maximum temperature in quench

Tem

per

atu

re (

K)

Time (s)

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.90

0.01

0.02

0.03

0.04

0.05

0.06Coil resistance in quench

Res

ista

nce

(O

hm

)

Time (s)0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9

0

5

10

15

20

25

30

35Quenching coil voltage

Vo

ltag

e (V

)

Time (s)

Preliminary

No quench heaters seem to be necessary

Page 37: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

MCBXFA: No damping resistance included

37

0 0.2 0.4 0.6 0.8 1 1.2 1.40

200

400

600

800

1000

1200

1400

1600Current decay in quench

Cu

rren

t (A

)

Time (s)0 0.2 0.4 0.6 0.8 1 1.2 1.4

0

50

100

150

200

250Maximum temperature in quench

Tem

per

atu

re (

K)

Time (s)

0 0.2 0.4 0.6 0.8 1 1.2 1.40

0.1

0.2

0.3

0.4

0.5

0.6

0.7Coil resistance in quench

Res

ista

nce

(O

hm

)

Time (s)0 0.2 0.4 0.6 0.8 1 1.2 1.4

0

50

100

150

200

250

300

350

400

450Quenching coil voltage

Vo

ltag

e (V

)

Time (s)

Preliminary

Page 38: J. García, F. Toral (CIEMAT) P. Fessia (CERN) January, 26 th 2015

MCBXFA: Damping resistance = 0.3 Ω (0.1 s delay)

38

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.90

200

400

600

800

1000

1200

1400

1600Current decay in quench

Cu

rren

t (A

)

Time (s)0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9

10

20

30

40

50

60

70

80

90Maximum temperature in quench

Tem

per

atu

re (

K)

Time (s)

0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.90

0.005

0.01

0.015

0.02

0.025

0.03

0.035

0.04

0.045Coil resistance in quench

Res

ista

nce

(O

hm

)

Time (s)0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9

0

5

10

15

20

25Quenching coil voltage

Vo

ltag

e (V

)

Time (s)

Preliminary