CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno...

26
Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 CKM SCRF Cavity Microphonics Detuning Compensation and Thermometry Developments

Transcript of CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno...

Page 1: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

CKM SCRF Cavity

Microphonics Detuning Compensation and Thermometry

Developments

Page 2: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Contributors

• PPD– Leo Bellantoni

• Beams Division– Tim Berenc– Al Beutler– Helen Edwards– Moyses Kuchnir– John Reid– Allan Rowe

• Technical Division– Ruben Carcagno– Steve Helis– Timergali Khabiboulline– Andrezj Makulski– Roger Nehring– Darryl Orris

Page 3: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Some CKM SCRF Cavity Parameters

• Frequency: 3.9 GHz• Cells/cavity: 13• Cavity Length: 660 mm• Qext = 6 x 107

• Bandwidth (f/ Qext): 65 Hz

• Main Injector Cycle Time: 3 sec• Extracted Beam Duration per cycle: 1 sec

Page 4: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Detuning Tolerance Target

• To keep RF power requirements low, it is desirable to keep the resonance frequency within ~ 1/10th of the bandwidth:

• From Finite Element Analysis models, ± 6.5 Hz corresponds to ± 3.1 nm in a 13-cell CKM cavity length.

• Failure to achieve this detuning tolerance target would require de-Qing the cavity further to increase its bandwidth, thus increasing the RF power cost.

2

2/1)0( 41

∆=

=∆ ff

PP

f

comp HzGHzf 5.69.3 ±=

Page 5: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Piezo Actuator Selection

• For prototype studies, we selected the Piezo Actuator P-206-40 from Piezosystem Jena. Some of its parameters are:– Bare piezostack compatible with cryogenic operation in liquid helium.– Voltage range: -10V to 150V– Range of motion (room temperature): 80 µm. At 1.8 K: ~ 8 to 10 µm– Length: 90 mm– Stiffness: 12 N/µm– Maximum Load: 1000 N – Capacitance: 8500 nF

Page 6: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

3-cell prototype instrumentation

• 3-cell prototype showing location of piezo element plus thermometry rings.

• Piezo element was used both as a sensor and as an actuator.

Page 7: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Microphonics FFT – All Pumps OFF

Page 8: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Microphonics FFT – Low Amplitude(~ ± 100 Hz)

Page 9: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Microphonics FFT - High Amplitude(~ ± 550 Hz)

Page 10: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Microphonics – Dewar Support Modifications(Measurements by T. Khabiboulline, April 2003)

Page 11: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Piezo-RF Phase Error Transfer Function

Page 12: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Manual Detuning CompensationRF Phase Difference With and Without Piezo Actuator Compensation

12/9/02, 4:13 PM

-10.00

-5.00

0.00

5.00

10.00

15.00

20.00

25.00

0 0.5 1 1.5 2 2.5 3

Time (s)

RF

Phas

e D

iffer

ence

(mV)

With CompensationWithout Compensation

FFT of Uncompensated RF Phase Difference and Piezo Drive Signal

12/9/02

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

0 10 20 30 40 50 60 70 80 90 100

Frequency (Hz)

FFT

FFT Piezo Drive SignalFFT Uncompensated RF Phase Difference

Microphonics detuning was reduced from ± 375 Hz to ± 175 Hz. Manual compensation is difficult because frequency, amplitude, and phase must be adjusted. In addition, only one sine frequency was used to drive the piezo actuator.

Page 13: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Automatic Detuning CompensationAdaptive Feedforward Control

• LMS Algorithm

xn Adaptive LMS F IR F ilter

yn S en

dn

The output of the filter is: y(n)=wT(n) x(n)

Where w(n) = [w0 w1 … wM-1]T is the weight vector at time index n and x(n) = [x(n) x(n-1) … x(n-M+1)]T is the

. data vector of the M most recent input samples. The weight vector is adjusted each iteration according to equation:

w(n+1)=w(n) + 2u x(n)e(n)

Where u is a convergence factor the value of which affects the amount the weight vector is altered on each iteration.

Page 14: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Active Noise Cancellation with Adaptive LMS FilterConcept Demonstration

• The LMS filter was implemented to cancel noise from a source speaker in a duct using a compensating speaker.

• The algorithm was programmed in a real-time VxWorks operating system. The signals were acquired with a VME-based data acquisition hardware.

Page 15: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Noise Cancellation Results

Page 16: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Noise CancellationAdaptation Details

Page 17: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

LMS applied to CKM cavity(preliminary)

xnAdaptive LMS FIR

Filtery n

en

dn = 3.9 GHz

Piezo Cavity RF phase difference

RF phase difference sample

(taken while LMS is OFF and “replayed”)

• This approach assumes the microphonics spectrum remains more or less constant between samples.

• Samples of the microphonics spectrum can be taken while the beam is OFF and then replayed to provide Xn. However, RF power is required for this measurement.

Page 18: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

13-cell cavity tuner cross section

Page 19: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Path Forward

• Demonstrate automatic microphonics detuning compensation in the 3-cell prototype using an FPGA board programmed with the adaptive feedforward LMS algorithm.

• 13-cell cavity measurements in operating conditions (e.g., mechanical resonances, piezo-rf transfer function, uncompensated microphonics)

• Characterization of the high-load piezo actuator to be used in the 13-cell cavity.

• 13-cell cavity measurements automatic compensation: strategy, fine-tune algorithm, etc.

• Packaging for production.

Page 20: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Cavity Thermometry - General• Cavity surface thermometry is used to study local distribution of

various types of energy losses and identify defects.• Main types of cavity loss mechanisms:

– Thermal breakdown (related to surface magnetic field)– Field emission (related to surface electric field)

• The temperature sensing element is usually Allen-Bradley carbon resistors encased in epoxy to prevent excessive cooling of the thermometer by the helium bath.

• Fixed or rotating arrays of thermometers have been used.

Page 21: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Example: 1.5 GHz Cavity(Cornell)

Page 22: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

CKM Cavity Thermometry• Small Iris size (30 mm) makes it difficult to use the general approach

used in other cavities with Allen-Bradley carbon sensors. A smaller CERNOX sensor was used instead.

• The sensor was attached with epoxy to a spring-loaded G-10 stick, and an Indium half-sphere was glued to the tip of the CERNOX sensor and covered with Apiezon grease prior to installation to improve thermal contact.

Page 23: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

CKM Cavity Thermometry

Page 24: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Cavity Quench Thermometry

Quench Operation(10 KHz data acquistion)

1.6

1.7

1.8

1.9

2

2.1

2.2

2.3

2.4

2.5

2.6

0 50 100 150 200 250 300 350 400

Time (ms)

Tem

pera

ture

(K)

ABCD

1.6

1.7

1.8

1.9

2

2.1

2.2

2.3

2.4

2.5

2.6

110

Tem

pera

ture

(K)

Quench Operation(10 kHz Data Acquisition)

111 112 113 114 115 116 117 118 119 120

Time (ms)

ABCD

Page 25: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Cavity cw thermometry at two different polarizations

CW Data, Polarization Mode I, 0.5 uA RTD current

-0.01

0.04

0.09

0.14

0.19

0.24

0.29

0 2 4 6 8 10 12Time (s)

Tem

pera

ture

Diff

eren

ce (K

)

RTD1RTD2RTD3RTD4RTD5RTD6RTD7RTD8

T (t=0) = 1.79K

CW Data, Polarization Mode II, 0.5 uA RTD current

-0.01

0.04

0.09

0.14

0.19

0.24

0.29

0 2 4 6 8 10 12Time (s)

Tem

pera

ture

Diff

eren

ce (K

)

RTD1RTD2RTD3RTD4RTD5RTD6RTD7RTD8

T(t=0)=1.78K

Page 26: CKM SCRF Cavity€¦ · – Andrezj Makulski – Roger Nehring – Darryl Orris. Ruben Carcagno Proton Driver LRP Meeting 7/11/2003 Some CKM SCRF Cavity Parameters • Frequency:

Ruben Carcagno Proton Driver LRP Meeting 7/11/2003

Path Forward

• We need to scale up the thermometry system for the 13-cell cavity.

• Software for automatic data reduction and analysis has to be written.