MKE heating with and without serigraphy    

49
MKE heating with and without serigraphy C. Zannini and G. Rumolo Thanks to: T. Argyropoulos M. Barnes, T. Bohl, G. Iadarola

description

MKE heating with and without serigraphy    . C. Zannini and G. Rumolo Thanks to: T. Argyropoulos M. Barnes, T. Bohl, G. Iadarola. Overview. Review of the impedance for the SPS extraction kickers (MKE) Power loss estimation -Power loss calculation method - PowerPoint PPT Presentation

Transcript of MKE heating with and without serigraphy    

Page 1: MKE heating with and without serigraphy    

MKE heating with and without serigraphy

C. Zannini and G. Rumolo

Thanks to: T. ArgyropoulosM. Barnes, T. Bohl, G. Iadarola

Page 2: MKE heating with and without serigraphy    

Overview

• Review of the impedance for the SPS extraction kickers (MKE)

• Power loss estimation-Power loss calculation method-Application to the SPS extraction kickers

• Comparison with heating observations• Effect of the bunch distribution• Summary and Future Plans

Page 3: MKE heating with and without serigraphy    

MKE kicker

The unshielded kicker exhibits a significant ferrite heating

Page 4: MKE heating with and without serigraphy    

MKE kicker with serigraphy

Page 5: MKE heating with and without serigraphy    

Comparing MKE with and without serigraphy

f=45 MHz fingereffeff

Lm.f

c 4780

Page 6: MKE heating with and without serigraphy    

The simulation of the EM fields seems to confirm that we have a quarter-wavelength resonance

Comparing MKE with and without serigraphy

Page 7: MKE heating with and without serigraphy    

An accurate low frequency model

• Model of the serigraphy– Accurate geometry of the serigraphy– Accounting finite conductivity

• Low frequency simulations– Longer bunch length– Studies of convergence

• Fit of the ferrite properties at low frequency

Page 8: MKE heating with and without serigraphy    

An accurate low frequency model

3500510440 peakZ.QMHzf

Page 9: MKE heating with and without serigraphy    

Overview

• Review of the impedance for the SPS extraction kickers (MKE)

• Power loss estimation-Power loss calculation method-Application to the SPS extraction kickers

• Comparison with heating observations• Effect of the bunch distribution• Summary and Future Plans

Page 10: MKE heating with and without serigraphy    

Power loss estimation

The single bunch approximation is valid only for broadband impedance because does not account for coupled bunch.

p

p|| pZRepQfPWL 0

20

2202

Single bunch approximation

spectrumbunch

peNQ

PWLnPWL bunchSBA

Page 11: MKE heating with and without serigraphy    

Power loss estimation

p

p|| pZRepQfPWL 0

20

2202

Full calculation

spectrumbeam

pbuncheNnQ

PWLPWLFC

SBAbunchFC PWLnPWL Qf

fIfPWLPWL rsFCSBA

8 72 8 7272 8 72

25ns buckets

Page 12: MKE heating with and without serigraphy    

Overview

• Review of the impedance for the SPS extraction kickers (MKE)

• Power loss estimation-Power loss calculation method-Application to the SPS extraction kickers

• Comparison with heating observations• Effect of the bunch distribution• Summary and Future Plans

Page 13: MKE heating with and without serigraphy    

Spectrum for the 25 ns beam distribution

Qf

fIfPWLPWL rsFCSBA

Due to peak of the serigraphy, we carry out the full calculation of the power loss.

Page 14: MKE heating with and without serigraphy    

Low frequency components of the beam spectrum

40 MHz

Page 15: MKE heating with and without serigraphy    

Power loss of MKE with and without serigraphy for the 25ns SPS beam

Due to the resonance introduced by the serigraphy the single bunch approximation differs from the full calculation because it does not account for coupled bunch

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Power loss of MKE with and without serigraphy for the 25ns SPS beam

At σ=0.3 the PWL on the MKE without serigraphy is only 30% larger than the PWL on the MKE with serigraphy

MKEser

MKE

PWLPWL

Page 17: MKE heating with and without serigraphy    

Power loss of MKE with and without serigraphy for the 50ns SPS beam

Due to the resonance introduced by the serigraphy the single bunch approximation differs from the full calculation because it does not account for coupled bunch

MKEser

MKE

PWLPWL

Page 18: MKE heating with and without serigraphy    

Comparing the power loss of 25 and 50 ns beam

At σ=0.3 the PWL on the MKE without serigraphy is only 30% larger than the PWL on the MKE with serigraphy for the 25 ns beam and a factor 2 larger for the 50ns beam

At flat bottom the PWL on the MKE without serigraphy is expected to be a factor 3-4.5 smaller than the MKE with serigraphy for the 25 ns beam and a factor 4.5-6 smaller for the 50 ns beam

MKEser

MKE

PWLPWL

Page 19: MKE heating with and without serigraphy    

Overview

• Review of the impedance for the SPS extraction kickers (MKE)

• Power loss estimation-Power loss calculation method-Application to the SPS extraction kickers

• Comparison with heating observations• Effect of the bunch distribution• Summary and Future Plans

Page 20: MKE heating with and without serigraphy    

Methods for calculation of PWL and T/t

dttPWLtt

PWLt

t 2

112

1

Up to now we calculated the power loss in a regime with four batches circulating in the SPS. In order to compare with heating observation we need to consider the dynamics of the beam with the time

T. Argyropoulos

dttI

ttI

i icycle

12

1

We assume the intensity per bunch unchanged

Page 21: MKE heating with and without serigraphy    

Methods for calculation of PWL and T/t

Renormalizing to the intensity the power loss remains unchanged for 1,2 and 4 batches. This proves that to account the cycle effect we need to consider only the intensity change

Page 22: MKE heating with and without serigraphy    

Methods for calculation of PWL and T/ t

thCFPWL

tT

The power loss is assumed to be uniform distributed on the ferrite and the cooling system is not taken into account

thCPWL

tT

MKEser

MKE

MKEser

MKE

PWLPWL

TT

T. Argyropoulos

Up to now we calculated the power loss in a regime with four batches circulating in the SPS. In order to compare with heating observation we need to consider the dynamics of the beam with the time

"F is the cooling factor which is at least a factor of 2 (J. Uythoven et al, BEAM INDUCED HEATING OF THE SPS FAST PULSED MAGNETS, EPAC 2004)"

Page 23: MKE heating with and without serigraphy    

The front probe measures more or less the average temperature of the ferrite

Cooling test bench: ferrite temperatures at different probe positions

SPS Extraction Kicker Magnet Cooling Design M. Timmins, A. Bertarelli, J. Uythoven, E. Gaxiola AB-Note-2004-005 BT (Rev.2) TS-Note-2004-001 DEC (Rev. 2)

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43 C

28 C

23 C 4520

MKEser

MKE

TT

25 April-26 April: 25 ns beam Ecloud studies

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We assume a bunch length of about 18 cm with the 25 ns beam at flat bottom

4

MKE MKE

th

MKEser MKEser

th

MKE MKE

MKEser MKEser

T PWLt C

T PWLt C

T PWLT PWL

25 April-26 April: 25 ns beam Ecloud studies

G. Papotti

In very good agreement with the measured heating

MKEser

MKE

PWLPWL

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25 April-26 April: 25 ns beam Ecloud studies

dttI

ttI

i icycle

12

1

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25 April-26 April: 25 ns beam Ecloud studies

dttII

icycle

Each point is the integral of the intensity along the 25ns cycle

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WPWL

WPWLMKEserhourMD

MKEhourMD

21

86

14

14

1.8

0.45

4

MKE MKE

th

MKEser MKEser

th

MKE MKE

MKEser MKEser

T PWL Kt C h

T PWL Kt C h

T PWLT PWL

K.TKT MKEserMKE 5626

TM

KE =

19 [K

]

25 April-26 April: 25 ns beam Ecloud studies

G. Papotti

“The cooling is expected to reduce the heating at least of a factor 2 (J. Uythoven et al, BEAM INDUCED HEATING OF THE SPS FAST PULSED MAGNETS, EPAC 2004)"

dttI

ttI

i icycle

12

1

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25 April-26 April: 25 ns beam Ecloud studies

Deltat=3 hours

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WPWL

WPWLMKEserhourMD

MKEhourMD

100

400

3

3

8.3

2.1

4

MKE MKE

th

MKEser MKEser

th

MKE MKE

MKEser MKEser

T PWL Kt C h

T PWL Kt C h

T PWLT PWL

K.TKT MKEserMKE 3625

TM

KE =

11.5

[K]

TM

KE =

3 [K

]

25 April-26 April: 25 ns beam Ecloud studies

G. Papotti

“The cooling is expected to reduce the heating at least of a factor 2 (J. Uythoven et al, BEAM INDUCED HEATING OF THE SPS FAST PULSED MAGNETS, EPAC 2004)"

dttI

ttI

i icycle

12

1

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50 ns beam: statistics

LHC Fill T[MKE]/T[MKEser]

2728 4.5

2729 6

2732 4.5

2816-2817 5

2818 5

2836 6

2838-2839 5

2845 5

2847 5

505 .stdTT

MKEser

MKE

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50ns beam 8 of july: LHC Fill 2818

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50ns beam 8 of july: LHC Fill 2818

dttII

icycle

Each point is the integral of the intensity along the 50 ns cycle

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dttPWLtt

PWLt

t 2

112

1

WPWL

WPWLMKEserhourMD

MKEhourMD

20

119

8

8

2.5

0.42

6

MKE MKE

th

MKEser MKEser

th

MKE MKE

MKEser MKEser

T PWL Kt C h

T PWL Kt C h

T PWLT PWL

K.TKT MKEserMKE 36320

TM

KE =

7.5[

K]T

MKE

=1.

5[K]

50ns beam 8 of july: LHC Fill 2818

T. Argyropoulos

“The cooling is expected to reduce the heating at least of a factor 2 (J. Uythoven et al, BEAM INDUCED HEATING OF THE SPS FAST PULSED MAGNETS, EPAC 2004)"

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Deltat=1.3 hoursThe integral of the intensity along the 50ns cycle is almost constant

50ns beam 8 of july: LHC Fill 2818

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dttPWLtt

PWLt

t 2

112

1

WPWL

WPWL

MKEserhourMD.

MKEhourMD.

62

368

31

31

7.6

1.3

6

MKE MKE

th

MKEser MKEser

th

MKE MKE

MKEser MKEser

T PWL Kt C h

T PWL Kt C h

T PWLT PWL

K.TKT MKEserMKE 7110

TM

KE =

4.5[

K]T

MKE

=1[

K]

T. Argyropoulos

50ns beam 8 of july: LHC Fill 2818

“The cooling is expected to reduce the heating at least of a factor 2 (J. Uythoven et al, BEAM INDUCED HEATING OF THE SPS FAST PULSED MAGNETS, EPAC 2004)"

Page 37: MKE heating with and without serigraphy    

Overview

• Review of the impedance for the SPS extraction kickers (MKE)

• Power loss estimation-Power loss calculation method-Application to the SPS extraction kickers

• Comparison with heating observations• Effect of the bunch distribution• Summary and Future Plans

Page 38: MKE heating with and without serigraphy    

Effect of tails

221 22

2

sbSignsbSignes

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Effect of tails

Lobes due to the truncation. This situation is unrealistic but is one of the worst conditions for lobes. The decay in frequency is very slow.

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Effect of tails

The power loss on the MKE with and without serigraphy calculated with the truncated Gaussian starts to differ from the one calculated using the Gaussian distribution only for truncation below 2.5σ

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Effect of core profile

2

1sg

geAsf c

cc sscosAsf2

22

112

3 ssAsf pp

dssfN

dssfs

N

222 1

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Effect of core profile

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Effect of core profile

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Effect of core profile

20

20 2

21

1f

sff

sf

8540.cos 7446530.par

FWHM

222

2lns

s fwhm

BQM

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Effect of core profile

Page 46: MKE heating with and without serigraphy    

Overview

• Review of the impedance for the SPS extraction kickers (MKE)

• Power loss estimation-Power loss calculation method-Application to the SPS extraction kickers

• Comparison with heating observations• Effect of the bunch distribution• Summary and Future Plans

Page 47: MKE heating with and without serigraphy    

Summary• The peak due to the serigraphy was accurately characterized• A power loss calculation formalism was presented and applied

to the MKE kickers for the SPS 25 and 50 ns beam. The limitations of the single bunch approximation were discussed.

• The PWL ratio between the PWL on the shielded MKE and the unshielded MKE has been found in very good agreement with the measured heatings

• An attempt of calculation of the T/ t was presented and found to be in good agreement with the measured T/ t

• The dependence of the PWL with the bunch distribution was investigated

• The good agreement with respect to the beam induced heating observed in the machine is also a confirmation with beam of the SPS kicker impedance model

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Future plans: MD proposal• 25 ns at 30 cm

The model predicts that the power loss on the MKE without serigraphy is only a 30% larger with respect to the MKE with serigraphy (better after a technical stop)

• 50ns at injectionTo eliminate in the analysis the uncertainity due to the time evolution of the bunch length

• 25 or 50ns coasting beam“Static” situation that cuold be simply benchmarked with the model (ideally, because in reality bunch lengths and intensities will change in time)

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Thank you very much for your attention