Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V....

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Transcript of Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V....

Page 1: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.
Page 2: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Potential improvements of the PS 10 MHz cavities driving amplifier

G. Favia

Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C. Rossi

Page 3: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Overview

① The PS RF 10 MHz system

② The PS 10 MHz cavities driving amplifier

③ Improvements of the present system and goal of the upgrade

④ Next modifications

⑤ Concluding remarks

Page 4: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

The PS 10 MHz System

Page 5: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

The PS machine contains cavities operating at different frequencies. The 10 MHz cavities are the most important because they accelerate the bunches to the desired energy and perform the required beam gymnastic.

The 10 MHz cavities (10+1 double gap cavities tuneable from 2.8 to 10 MHz) are driven by amplifiers based on electron tubes (power up to 60 kW), for radiation hardness and power dissipation constraints.

PS High Level RF System

Page 6: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Ferrite loaded cavity

Gap voltage 0.5 - 10kVp

Frequency range 2.8 – 10 MHz

Tuning via bias current that saturates the ferrite

Ferrite loss resistance:22kΩ/gap @3MHz

10kΩ/gap @10MHz

RF amplifier adopting:

3xYL1056 tubes for predriver and driver

1xRS1084 in the final stage

Housed in the cavity base

Built in 1975, upgraded in 1988

10 MHz System

Courtesy of C. RossiCourtesy of C. Rossi

Page 7: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

𝑍𝐶𝐴𝑉′ =

𝑍𝐶𝐴𝑉

1+ 𝐴𝛽

¿𝐺𝐿∨¿|𝐴 · 𝛽|=1=0𝑑𝐵INSTABILITY ->

gain margin (GM)and

phase margin (PM)

LIMITS:

Delay introduced by cables and electronics 𝜏=

∆𝜑  ∆𝜔

= feedback factor

= A0 R = forward gain

A. Gallo, Beam Loading and Low-Level RF Control in Storage Rings (CAS 2005)

The impedance of the 10 MHz cavity as observed by the beam would be several kΩ per gap due to the ferrite losses and the final tube anode resistance. This high impedance would lead to strong beam loading.

Wideband Negative Feedback

∠𝐺𝐿=−180 º

Page 8: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

The PS 10 Mhz Cavities Driving Amplifier

Page 9: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

LOAD IMPEDANCE TRANSFORMATION FROM 50Ω TO 200Ω(1:4)

FREQUENCY TUNING VIA A DC CURRENT

180° PHASE SHIFT FOR THE LOCAL FEEDBACK

GDELAYGROUP

BW= 1.25 MHz

BW= 3.5 MHz

Frequency

BW = 1.2 MHz

BW = 65 kHzLG=21 dB

Amplifier Description

Page 10: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Improvements of the Present System and Goal of the Upgrade

Page 11: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

STAGE GAINOld configuration

GAINNew configuration

Predriver 11.1 dB 12.76 dB

Driver 26.7 dB @3MHz24 dB @10MHz

28.5 dB @3MHz26 dB @10MHz

Final 42.5 dB @3MHz38.3 dB @10MHz

44.5 dB @3MHz40.5 dB @10MHz

TOTAL INCREASE OF GAIN: ~4dB IN THE FIRST TWO STAGES

~2dB IN THE FINAL STAGE

In order to get higher tubes transconductance and hence higher open loop gain, the working point of the tube has been modified.

Working Point Change

Page 12: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Starting point: GL=21 dB

1. β has been increased by 3 dB → GL= 24 dB→ that means more input power needed (but still achievable);

2. A has been increased by 6 dB → GL=30 dB→ that means keeping the same input power.

The additional 6 dB have been distributed in this way:Starting from GL =24 dB→ 3 dB used for decreasing the cavity impedance;→ 3 dB used for reducing the total group delay by acting on the local feedback or implementing

hardware modifications; → the grid resonator has been replaced in order to improve the stability of the system.

GL=27 dB + stability

Upgrade Goal

3 MHz 10 MHz

Page 13: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Final Grid Resonator Studies• Old resonator (4L2 ferrite): stray capacitance and leakage inductance, high losses at 10 MHz.

• New resonator prototypes: Transmission line solution ADVANTAGES:• It limits stray capacitance and leakage inductance• The combination of parallel and orthogonal bias guarantees less losses at 10MHz .

DISADVANTAGE:• too high current and overheating• 4L2 ferrite is not available in toroids shape

3 MHz 10 MHz

DRIVERLOAD

194 Ω 120 Ω

Page 14: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

New Grid Resonator Tuneable resonator coil :• two ferrite rings 4L2• 6 sections of RF winding, two 8- shaped turns and. • 6 biasing sections, each one has ten O-shaped turns. 200Ω load transformer :• ferrite ring wounded by a coaxial cable.Inverter :• a ferrite ring wounded by a coaxial cable carries the

local feedback and the phase inverter transformer.3 MHz 10 MHz

DRIVERLOAD

186 Ω 177 Ω

HIGH FIELD TESTS

10 MHz3 MHz ≈15%10 MHz

V V

Page 15: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Other ImprovementsThe connection between the resonator and the grid of final has been improved

Three 3.3 nF capacitors in parallel reduce the equivalent inductance of the connection

new connectionold connection

Page 16: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

R 23425

R 2065

L241m

R 183100

0

C3100p

R1841.5k

R 185

4 . 7 k

C 794 . 7n0

C80147p

R 105

00 0

R 1865

Rin2

50

R 1

5

C1100pF

LOAD1

50

R3

1.5k

+-

R 2

4 . 7 k

0

C 2

4 . 7nF

0 0

L11m H

R 4100

U g1_PR E 1

0

R 55

R 65

Loop Gain Measurements

R 23425

R 2065

L241m

R 183100

0

C3100p

R1841.5k

R 185

4 . 7 k

C 794 . 7n0

C80147p

R 105

00 0

Page 17: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

The summing point equivalent circuit coherently reproduces the real input stage in the range of frequency where the margins are evaluated

The loop gain can be directly evaluated.Previously calculated as:

Loop Gain Measurements

Page 18: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Local Loop Stability Margins Evaluations

LOCAL LOOP 3 MHz

OL=33.5 dBCL=26 dB

1 + Af= 7.5 dB Af = 2.5 dBmϕL,R=180 – |ϕ (0 dB)|≈ 145°

mGL(Af=180) = 17 dBmGL(Af=180) > 12 dB

0 dB 0 dB

180 °

→180 °

33.5 dB

26 dB

Page 19: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

LOCAL LOOP 10 MHz

OL=32.8 dBCL=26 dB

1 + Af= 6.8 dB Af = 1.25 dB

mϕL=180 – |ϕ (0 dB)|≈ 165°mϕR=180 – |ϕ (0 dB)|≈ 100°

mGL(Af=180) > 20 dBmGR(Af=180) ≈ 20 dB

0 dB 0 dB

→180 °

←180 °

32.8 dB

26 dB

Local Loop Stability Margins Evaluations

Page 20: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

TOTAL LOOP 3 MHz

OL=69.5 dBCL=42.8 dB

1 + Af= 26.7 dB Af = 26 dB

mϕL=180 – |ϕ (0 dB)|≈ 80°mϕR=180 – |ϕ (0 dB)|≈ 52°

mGL(|Af|Af=180) = 11 dBmGR(Af| Af=180) = 17 dB

ϕ(3 MHz)= -12°

69.5 dB

42.8 dB

0 dB 0 dB

180 °

180 °

Total Loop Stability Margins Evaluations

INPUT POWER REQUIRED FOR 10 kVP

80 W

Page 21: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Instability at 10 MHz

TOTAL LOOP 10 MHz

At 10 MHz the system resonant peak shifts when the loop is closed. If the resonator is tuned at 10 MHz the closed loop curve is asymmetric.

The resonator has to be tuned at higher frequency to get the stability

Page 22: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

TOTAL LOOP 10 MHz

OL=64.3 dBCL=42.1 dB

1 + Af= 22.2 dBAf = 21.21 dB

mϕL=180 – |ϕ (0 dB)|≈ 70°mϕR=180 – |ϕ (0 dB)|≈ 100°

mGL(|Af|Af=180) > 25 dBmGR(Af| Af=180) ≈ 12 dB

ϕ(10 MHz)=14°

Δϕ(3-10 MHz)= 26 °

64.3 dB

42.1 dB

0 dB 0 dB

180 °

←180 °

Total loop stability margins evaluations

INPUT POWER REQUIRED FOR 10 kVP

120 W

Page 23: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Next Modifications

Page 24: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

The phase shift is caused by the input capacity of driver stage and the 50 Ω predriver load

Reduce the predriver load from 50Ω to 33Ω

Next Modifications

POSSIBLE SOLUTION:

Act on the compensating circuit in parallel to the predriver load to reduce the phase shift introduced by the predriver

Reducing the predrived load from 50Ω to 33Ω is beneficial at 10 MHz but could make the 3MHz responce less symmetric

3 MHz

10 MHz

Phas

e ( °

)G

ain

(dB)

Frequency (Hz)

50 Ω33 Ω

Phas

e ( °

)G

ain

(dB)

Frequency (Hz)

50 Ω33 Ω

Page 25: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Concluding Remarks

Page 26: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Higher amplifier gain is achievable without complete re-designing;

Up to 9 dB of additional loop gain have been demonstrated;

A stable operation with additional 6 dB of loop gain at 3 MHz can be achieved with an achievable input power by implementing few changes to the amplifier

Measurements with high voltage will be performed in order to verify the output rensponse stability ;

New modifications will be implemented in order to get higher loop gain with less input power at 10MHz;

The overall feedback pickup will be moved from the anode of the final tube to the cavity, since the cavity acts as a good bandpass filter;

Asymmetries in the distribution of the beam induced voltage in the two cavity gaps will be analyzed;

The possibility to replace the first two stages with solid state amplifiers, or to clearly change technology for the cavity-amplifier system (wideband Finemet© cavity) will be investigated, if necessary.

Summary

Next Steps

Page 27: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

THANK YOUFOR YOUR ATTENTION

Page 28: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

Spare Slides

Page 29: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.
Page 30: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.
Page 31: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.
Page 32: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

The LHC 25ns Cycle In The PS (pre-LS1)

h = 7

Eject 72 bunches

Inject 4+2 bunches

gt

r

h =

84

h = 21 Instability

In the PS different multi-bunch beams are generated: 25, 50, 75 ns LHC physics beams. The 25 ns LHC physics beam is referred to as ‘nominal’ LHC beam.

Split in four at flat top energy

Courtesy of H. Damerau & L. Ventura

Triple splitting after 2nd injection

• LIU PROJECT: New LHC beam planned for the LIU project -> Increased intensity ppb at extraction

Page 33: Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.

STATIONARY BEAM LOADING

TRANSIENT BEAM LOADING

In stationary conditions, Vg must compensate Vb , to keep Vt at the desired value, providing an extra driving power or detuning the cavity.

In transient situations the voltage Vt will vary. It happens in many circumstances, such as at the injection or when the ring is not filled uniformly. The transient beam loading experienced by the bunch is the result of different spectral components besides the ones at the RF frequency.

Beam Loading