44
Crab Cavity Workshop 9-11 Dec 2013 CERN Geneva Power Amplifiers & Fundamental Power Coupler

Crab Cavity Workshop 9-11 Dec 2013 CERN Geneva

Embed Size (px)

DESCRIPTION

Power Amplifiers & Fundamental Power Coupler. Crab Cavity Workshop 9-11 Dec 2013 CERN Geneva. Contents. FPC Initial design February 2013 Arcing in air line New design December 2013 Test boxes designs Schedule PA Tetrode amplifier Driver amplifiers Power supplies - PowerPoint PPT Presentation

Citation preview

Page 1: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

Crab CavityWorkshop

9-11 Dec 2013CERN Geneva

PowerAmplifiers

&Fundamental

PowerCoupler

Page 2: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 2

Contents

• FPC– Initial design February 2013– Arcing in air line– New design December 2013– Test boxes designs– Schedule

• PA– Tetrode amplifier– Driver amplifiers– Power supplies– Circulator & integration

9-11 December 2013, CERN

Great thanks to: Antoine Boucherie

Sébastien CalvoMany MME colleagues

Great thanks to: Charles Julie

Page 3: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 3

FPC – initial design

• 400 MHz 50 kW CW FPC

• We agreed on a coaxial lineOD 62 mm / ID 27 mm

• We designed a coaxial disk window scaled to the recent SPL coupler developed at CERN– Titanium flange– Al2O3 97.6% ceramic– Copper tube

9-11 December 2013, CERN

Page 4: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 4

FPC – initial design

• 400 MHz 50 kW CW FPC

• We agreed on a coaxial lineOD 62 mm / ID 27 mm

• We designed a coaxial disk window scaled to the recent SPL coupler developed at CERN– Titanium flange– Al2O3 97.6% ceramic– Copper tube

9-11 December 2013, CERN

Titanium flange

Copper tube

Ceramic

Page 5: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 5

FPC – initial design

9-11 December 2013, CERN

Body

DT flange

Window flange

• Coupler body– Massive copper– 316 LN Stainless Steel

flanges on both sides

• Monitoring ports– 1 port for vacuum gauge– 1 port for e- monitoring– 1 port for arc detector

Page 6: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 6

FPC – initial design

9-11 December 2013, CERN

Vacuum gauge

Arc window

e- antenna

• Coupler body– Massive copper– 316 LN Stainless Steel

flanges on both sides

• Monitoring ports– 1 port for vacuum gauge– 1 port for e- monitoring– 1 port for arc detector

Page 7: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 7

FPC – initial design

• From this window we have a coaxial to WG WR2300½H transition without doorknob

• There is also a DC capacitor included in the design for DC polarization

9-11 December 2013, CERN

Page 8: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 8

SPL experience – arcing in air side• This SPL coaxial disk is very similar

• 100 / 43.5 mm coaxial line

• Operating 704 MHz 2 ms – 50 Hz up to 1 MW SW all phases

• At 650 kW SW with a particular phase, we started to arc in the air side around the ceramic, along the coaxial line and in the waveguide

• We were limited to 500 kW SW

9-11 December 2013, CERN

Page 9: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 9

SPL experience – arcing in air side

9-11 December 2013, CERN

Page 10: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 10

Coaxial straight line maximum rating

9-11 December 2013, CERN

Page 11: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 11

New crabFPC design

9-11 December 2013, CERN

Page 12: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 12

Coaxial vacuum line

We kept the agreedOD 62 mm / ID 27 mm

coaxial lineon the cavity side

9-11 December 2013, CERN

Page 13: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 13

Conical vacuum body

We designed a conical vacuum line to increase

the diameter of the ceramic in order to avoid

arcing on the air side

The goal is to have the air side size as large as possible to avoid arcing

9-11 December 2013, CERN

Page 14: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 14

Ceramic

OD is increased to100 mm to reduce the

risk of arcing

We have chosen a very thick ceramic of 20 mm to make this coupler as

robust as possible

9-11 December 2013, CERN

Page 15: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 15

Pseudo conical air body

The extension from the ceramic to the waveguide is

pseudo-conical in order to increase arcing

robustness

9-11 December 2013, CERN

Page 16: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 16

Pseudo conical air body

This air extension is cooled with forced air

This ensures a correct cool down to

compensate losses of the thick ceramic

This also reduces the arc development by quickly replacing any ionising air (tips coming from X-ray

tube specialist)

9-11 December 2013, CERN

Page 17: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 17

Antenna water cooling

To ensure a ‘stable’ coupling element

position the antenna is water cooled

Against cern’s rule:no soldering in between

water and vacuum

No other way to do it

9-11 December 2013, CERN

Page 18: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 18

Electron Beam Welding

To avoid any water into the RF path the antenna

is EBW

This implies huge integration constraints

9-11 December 2013, CERN

Page 19: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 19

Vacuum gauge

In order to monitor the outgassing around the ceramic and to protect

the coupler in operation and while RF processing

a vacuum gauge is mandatory

9-11 December 2013, CERN

Page 20: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 20

Vacuum gauge

It has been oriented to reduce to its minimum

its footprint

The size of the pipe is a compromise between

vacuum reading speed & RF shielding

9-11 December 2013, CERN

Page 21: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 21

Arc window &e- monitor

We removed the arc detector window and the

e- antenna to simplify integration

Arc protection will be from the top of the

waveguide looking into the direction of the

ceramic

9-11 December 2013, CERN

Page 22: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 22

Doorknob free transition

The coaxial to WR2300½H waveguide transition is a plug and

play without a doorknob and with an integrated

step waveguide

It will be mono-bloc from 3D print to avoid any

arcing

9-11 December 2013, CERN

Page 23: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 23

DC capacitor

The DC capacitor is included with finger contact all around to

reduce to its minimum the constraint given to

the ceramic

9-11 December 2013, CERN

Page 24: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 24

Three designs

Three designsfully compatible

with the only difference:coupling element

9-11 December 2013, CERN

Page 25: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 259-11 December 2013, CERN

Four air & waveguide lines will be built

Two for the machine Two for the test bench

Eight window lineswill be built in order to

provide six couplers

Page 26: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 269-11 December 2013, CERN

400 MHz

S11 –30 dB

300 MHz 500 MHz

0 dB

-30 dB

-60 dB

Page 27: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 27

Test boxes• Three test boxes will be built allowing

the preparation of pair of couplers

• They will be two plates and one special shim, with two helicoflex seals

• They will be customized regarding the coupling element

• We will not copper plate them, easier and quicker

• They will be water cooled

9-11 December 2013, CERN

Page 28: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 28

Integration• As already asked in August, the

DT length is a mandatory dimension needed to calculate– Antenna length– Test boxes– The space for integration in LSS4

• Key parameter is the distance between beam axis and the water inlet on the top of the waveguide

• Cryomodule design must take it into account

9-11 December 2013, CERN

2308

max

imum

1200

DT 1108

Courtesy ofThierry Renaglia

Giuseppe FoffanoOfelia Capatina

Page 29: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 29

Integration• As already asked in August, the

DT length is a mandatory dimension needed to calculate– Antenna length– Test boxes– The space for integration in LSS4

• Key parameter is the distance between beam axis and the water inlet on the top of the waveguide

• Cryomodule design must take it into account

9-11 December 2013, CERN

Courtesy ofThierry Renaglia

Giuseppe FoffanoOfelia Capatina

Page 30: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 30

Schedule December 2012 (Fermilab)

9-11 December 2013, CERN

Cavities to be installed in SPS in December 2015 Cryostat fully tested Q3 2015 Cryostat fully dressed Q2 2015 Couplers available for cryostat Q1-2015 Couplers RF processed 50 kW SW CW all phases Q4-2014 Couplers assembled in clean room onto test box Q2-2014 Special processes FPC + Test Box (Cleaning, Brazing, EB welding, Gold

plating, Ti coating) completed Q1-2014 All couplers + Test Box parts machined Q4-2013 All missing raw material delivered Q2-2013 All missing raw material ordered Q1-2013 Design completed February 2013 (+ Test Boxes)

2013 2014 2015 2016

Design FPC RF processed In LSS4

Page 31: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 31

Schedule December 2013 (CERN)

9-11 December 2013, CERN

Cavities to be installed in SPS in December 2016 Cryostat fully tested Q3 2016 Cryostat fully dressed Q2 2016 Couplers available for cryostat end Q2-2015 Couplers RF processed 50 kW SW CW all phases Q2-2015 Couplers + DT assembled in clean room onto test box Q1-2015 Special processes FPC + Test Box (Cleaning, Brazing, EB welding, Gold

plating, Ti coating) completed Q4-2014 All couplers + Test Box parts machined Q3-2014 All missing raw material delivered Q2-2014 All missing raw material ordered Q1-2014 Design completed February 2014 (+ Test Boxes NEED DT definition)

Design → FPC RF processing LSS4

2014 2015 2016 20172013

DT →

Page 32: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 32

Tetrode Amplifiers• The old 400 MHz amplifier has

been refurbished from SPS

• Unfortunately, no water in our test bench this year due to LS1

• Water will be ok by April 2014

• From old tests : 40 kW CW

• With a better cooling we should be able to go up to 50 kW if needed (not guaranteed)

9-11 December 2013, CERN

Page 33: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 33

Circulators• We decided to use the LHC 400 MHz 330 kW circulators

• We will buy two units and LHC team will provide one for test bench

• Drawback : they are huge

• This induces integration difficulties

• Amplifiers must be on the table

• We will design compact loads

9-11 December 2013, CERN

Page 34: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 349-11 December 2013, CERN

Courtesy ofThierry Renaglia

Giuseppe FoffanoOfelia Capatina

Circulators

Tetrode amplifier

Compact load

Page 35: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 35

Driver amplifiers• SSA in the power range between 2 kW and 4 kW

• 17 companies contacted

• 10 qualified

• Offers received, off the shelves SSA

• On-hold awaiting Tetrode amplifier test results in order to correctly define the output power level regarding tetrode amplifier gain

• They will be close to the LLRF racks in ECX4

9-11 December 2013, CERN

Page 36: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 36

Power supplies

• Existing one can be operated in test stand

• Two new systems have to be built for BA4

• Could be one HV power converter for the two amplifiers to reduce the cost

9-11 December 2013, CERN

Page 37: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 37

Conclusion

• Coupler design close to completion

• DT length must be defined asap

• Test boxes simulations have to be completed

• Tetrode amplifier still to be tested

• Integration difficult, however feasible

• Schedule … optimistic !

9-11 December 2013, CERN

Page 38: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 389-11 December 2013, CERN

Thank youvery much

For yourAttention

Page 39: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 39

Spare slides

9-11 December 2013, CERN

Page 40: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 40

SPL experience – arcing in air side

• Arcs are moving towards the RF source

• The explanation is probably the brazing shapes reducing the voltage breakdown capability along the ceramic

• Were not included in simulations

9-11 December 2013, CERN

Perfect in drawing & simulation

Brazing shapes

Page 41: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 41

FPC – initial design

• We launched the purchasing of ten– Ceramics– Titanium flanges– Copper tubes

• Titanium & copper are already delivered

• Ceramics are about to be delivered

9-11 December 2013, CERN

Page 42: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

LHC-CC13, 6th LHC Crab Cavity Workshop, Eric Montesinos, CERN-RF 429-11 December 2013, CERN

50 kW

400 MHz

OD 120 mm

100 kWOD 200 mm

400 MHz

50 kWOD 115 mm

100 kWOD 180 mm

Page 43: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

43

Key R&D resultsInner line with specific RF contact

• Air cane ensuring 1 MW RF contact :

1. Inner ceramic is brazed with a stainless steel nut

2. Air cane is built with a specific bolt

3. Air cane is screwed compressing springs

4. Springs ensure a good RF contact

1.

2.3.

Page 44: Crab Cavity Workshop 9-11  Dec 2013 CERN  Geneva

44

Key R&D resultsTest box

• All in one, only two covers conditioning test box

• Pros :– Easier (not easy) copper sputtering– Self supporting shape– Easily cleanable for SRF needs, can be

used for several sets of coupler (if large series : SPL, ESS, …)

• Cons :– Helicoflex faces to be very well

prepared– Self-supporting structure : heavy

weight