1. CERN Chopper Status LINAC4 – approach to the problem, past experience at CERN and proposal for ESS specific conditions F. Caspers CERN, HIPPI 08 meeting October 29 th, 2008 And shown again in Bilbao Jan. 26 th 2015 Bilbao workshop Jan 2015 1

2. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 2   Introduction CERN chopping scheme Layout Technical requirements   Evolution of the SPL chopper Modifications in 2005 Status by September 2006 What happend since end of 2006 Status by April 2008 Some photos What is still to be done  Drivers Status  Acknowledgements Contents Most of these slides were already shown in May 2008 at the WP4 meeting

3. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 3   Superconducting Proton Linac (SPL)   Fast beam chopping at E kin = 3 MeV ; thus  is about 8% Fast chopper required to establish desired beam pattern SPL Layout  RFQ: Radio frequency quadrupole  DTL: Drift tube linac  CCDTL: Coupled cavity DTL  PIMS (PI-Mode Structure)   = 0.65,  = 0.92 : superconducting cavities

4. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 4 8*2.84 ns ( 44 MHz)   Most demanding scheme for SPL operation: cutting out three bunches out of eight repetition rate 44 MHz bunch spacing 2.84 ns ; 10 to 90% rise and fall time required < 2 ns CERN Chopping Scheme

5. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 5 Chopper off   Chopper line lattice designed such as to magnify the kick from the chopper; this reduces required kick field   The chopper plates have to be installed in the quads; this saves length and reduces space-charge related emittance growth Chopper Line (1) Chopper on Kick-magnifying quad

6. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 6 Chopper Line (2) chopper beam dump bunching cavities

7. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 7   The chopper plates are no longer DC-wise floating (no more triaxial mode of operation)   Now we have a coaxial instead of a triaxial chopper structure   The triaxial version was meant for simultaneous dual mode of operation, i.e. 0 to 10 MHz: electrostatic deflector, above 10 MHz travelling wave mode   Removal of isolating units both in water cooling circuits and coaxial driving lines Modifications in 2005

8. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 8   Initially samples of the meander lines were produced at CERN   While all parameters were basically ok (electrical, vacuum), reproducibility of certain electrical parameters (electrical length, match) was not always perfectly satisfactory   After the accomplished proof of principle with CERN technology, a supplier that can well control all the process parameters was needed; a possible change in technology is not a problem as long as the key properties are preserved   Kyocera was eager to enter in a cooperation with CERN and willing to adapt their technology to our needs   The plate that was recently furnished compared well in all aspects with the best CERN samples and we hope that the promised good reproducibility will show up in reality Meander lines

9. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 9   Technological differences between the CERN and Kyocera meander structures: Meander line: Technology CERNKyocera CERN orders from Wesgo (D) ceramic plates with fixation holes and 10 to 15  m thick homogeneous MoMn layer (fired at 1400 C in hydrogen atmosphere Kyocera produces the alumina plates in-house. Then a meander pattern is created in thick film silver paste of about 10 to 15  m thickness. This thick film silver paste has after firing a much higher resistivity than bulk silver (factor 5 to 10) The meander structure is etched into the MoMn layer. Afterwards a 1 to 2  m thin-film layer of Ag is attached by sputtering. Onto the Ag thick-film layer 30 to 40  m copper are deposited electrochemically In a final step this silver-coated MoMn layer gets another 30  m silver by electrochemical deposition Finally 1 to 2  m of Au are applied for good contacts and protection against oxidation In the meantime (october 2008) I learned that it is possible to produce nonmagnetic Nickel layers by adding 18 % of phosphor [F.C.]

10. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 10 Metallize printing (Ag thick-film) Firing Cu Plating Resistance Testing Final inspection Packing Machining Ceramic incoming inspection Au Plating CERAMIC PLATE Process Flow RF Property Testing Machining Electrode for electrochemical deposition removed by grinding Grinding Area Courtesy: Kyocera

11. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 11   First meander line plate from Kyocera were received in June 2006 but it turned out that the attenuation was too high   In the second iteration the technological parameters were properly adjusted and the last sample was very satisfactory   After extensive electrical tests this single plate was installed in the chopper tank   Vacuum, leak and heat tests performed successfully Status by September 2006

12. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 12 Electric Measurements: Transmission Attenuation   Measurements performed on single chopper plate with an image plane 10 mm above the line’s surface to simulate the presence of a second plate   Frequency domain transmission   A DC resistance of 1.1  was measured, which agrees very well with the low-frequency limit of the measured attenuation   3 dB bandwidth 940 MHz. If there was no phase distortion the rise time would be   All rise times quoted are 10 to 90% values Attenuation over one chopper plate Generator bandwidth

13. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 13 Transmission Step Response   Response for 0 to 700 MHz low pass step function (Kaiser Bessel weighting function with  = 6)   Comparison between a measurement with and without the image plane. Due to the high electric field energy in the alumina the kick field does not change much when the symmetry is broken   Measured rise time t rm = 1.771 ns, to be compared with t ri = 1.407 ns of input pulse; structure rise time   This is a conservative estimate of t r since the t ti is rather short and we get into the highly dispersive region of the response

14. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 14 Phase Distortion   From the measured phase without image plate the electrical delay of 16.73 ns (linear term) was removed   With image plane (realistic configuration) the electrical length was 16.83 ns, within 0.1 ns of the required value   The remaining phase is not flat as for a dispersion-free line; thus we have phase distortion   The phase distortion is due to coupling between adjacent lines in the meander structure. This coupling increases quickly with frequency like in a microstrip directional coupler   In an ordinary first-order low-pass the 45 degree points coincide with the 3 dB points. Here they are at 375 MHz, i.e. much lower than the 3 dB points Generator bandwidth Phase without image plane

15. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 15 Reflection   Very good impedance match of meander line to 50  : reflection in frequency domain of the order of -30 dB below 500 MHz   These data were measured on a test jig consisting of a single plate with SMA connectors fixed on either side Generator BW

16. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 16 Reflection Step Response   Response for 0 to 700 MHz low pass step function   S 11 very small, of the order of 0.02 which is another indication of good match   The line impedance is not perfectly constant over the meander length as can be seen from the bump at t = 10 ns.   Towards the end of the line an apparent increase in line impedance can be seen. This is an artifact caused by the lossy line; could be corrected numerically Twice the line length of ¼17 ns

17. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 17 Tuning of Electrical Length   It was tried to adjust the electrical delay of a chopper plate by modifying the metal ground plane   Cutting a longitudinal groove into the ground plane reduces the effective  and thus increases the group velocity on the line. Since the variation in line impedance is over distances much shorter than the wavelength, the other electrical properties should not be affected much   For two 5 mm wide and 3 mm deep grooves a 5% decrease in the electrical length was found on a CERN plate Generator bandwidth

18. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 18 What happend since end of 2006 ? (1)   We have seen that the originally used aluminum support plates for the alumina ceramic are not usable since they liberate internal stress when heated and show considerable deformation ( up to several 100 micron); this has even led to the destruction of ceramic substrates when mounted (fortunately only old ones, which we were allowed to destroy)   This deformation is a very critical issue since the thermal contact betwen the ceramic plate and the metal support depends strongly on the small vacuum gap between the ceramic and the metal.   In fact this point has been subject of many discussions and the heat transfer between the ceramic and metal plate is essentially an electromagnetic tunneling effect !   The wavelength corresponding to room temperature is about 10 micron we the average space between metal and ceramic plate has to be below a few microns in order to meet the tunneling condition (similar to a microwave waveguide below cutoff signal transmission)

19. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 19 What happend since end of 2006 ? (2)   Thus it was decided to replace those aluminum plates by stainless steel plates which are heat treated (to release all internal stresses) and copper coated (without using nickel as intermediate layer [magnetic field!) and finally having a flash of gold to prevent oxydation.   The copper coating towards the ceramic layer is required for keeping losses of the image currents from the microstrip structure within reasonable limits.   One may raise the question about degradation of thermal conductivity due to the use of stainless steel The anser is that this completely irrelevant since the thermal impedance of the vacuum gap is by far the dominating contribution.This has been shown experimentally in vacuum in 2006. If one would solder/braze the ceramic plate directly onto the metal support the thermal resistance would reduce by more than factor of 30. This is relevant and also under discussion in the frame of applying this concept at GANIL

20. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 20 What happend since end of 2006 ? (3)   We also noticed that due to changes in production technology at Kyocera (now all parameters are well under control and production is reproducible) certain samles did not meet out specs and we had to return them.   As a consequence we found a considerable scatter (up to 1.5 ns) in electrical delay as well as a systematic offset between the different ceramic plates which were delivered over the last 3 years.   Thus we had to apply means in reducing the scatter and getting the mean value of the delay right (16.7 ns nominal)   For this problem we decided to apply the „groove“technique for fine tuning, which of course only works on one direction i.e. reducing the el. delay.   In this context the question comes up: How is the electrical delay (which is frequency dependent, see privious slides) exactly to be defind? Do we take the el.delay at low frequencies or at 100 MHz or at 200 MHz ? Or do we refer to the 50% point of the rising slope of the step excitation ?

21. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 21 Transmission Attenuation Status April 2008 Transmission Attenuation Status April 2008 Loss values of 1 db at 200 Mhz are ok. and consistent with previous data.

22. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 22 Transmission Step Response Status April 2008 We will place plate1 and plate2 (red and green trace) into one chopper unit as they match rather well (c.f. 50% point) and plate 3 and plate 4 into the other unit

23. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 23 El.Delay, Status April 2008

24. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 24 Reflection (frequency domain) Status April 2008

25. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 25 Reflection (time domain, step response) Status April 2008 Note that for the blue and the green trace the char. impedance is slightly too low (refl factor -2 %) and for the red trace is slightly too high (+2 %)

26. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 26 Some photos (1) Rear side with water cooling circuit and RF connectors for rigid coax lines to the vacuum feedthrough grooves Note, that the grooves are good for venting (vacuum) the confined space between the ceramic plate and the metal support

27. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 27 Some photos (2)

28. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 28 What is left to be done  Final assembly of the chopper plates and the tanks …..done by now (October 2008) the chopper tanks are already in the beamline under construction.  Final vacuum test…done by now (October 2008)  Final electrical test (DC high voltage and DC high current) under vacuum; such tests were done already 2 years ago, but not on the same ceramic plates  DC tests with beam (DC bias voltage on the plates with open termination = Static deflection)  RF power tests under vacuum without and with beam when the pulser is available.  Production of spare quadrupoles !  Whatever else I might have forgotten….

29. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 29 Drivers status FID Technology Pulsers  Positive and negative units have been delivered and characterized.  Units succesfully tested at 1MHz, 1ms burst and 50Hz repetions rate for two weeks continuos operation.  Reliability problems due to incorrect triggering could be highligted.

30. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 30 Drivers status Achieved parameters PARAMETERREF.SPEC.ACHIEVED Output voltageV out 700 V670 V Load impedanceZ out 50  OK Pulse lengthT Wout 8 ns to 1  s OK Minimum rep. freq.f min Single pulseOK Maximum burst lengthTBTB 1 ms Maximum burst rep. freq.f Bmax 50 Hz

31. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 31 Drivers status Parameters to improve (1) PARAMETERREF.SPEC. ACHIEVED Minimum off pulse time T off dep. on T Wout T off dep. on rep. freq. T off 14 n No 40 ns OK Maximum repetition frequencyf max 45 MHz15 MHz Rise time (10 % - 90)TRTR <2 ns<2.5 ns Rise time (3 % - 90)T RR <2.5 ns<3 ns Fall time (90 % - 10)TFTF <2 ns<3 ns Fall time (90 % - 3)T FF <2.5 ns<3.7 ns Max. voltage between two pulses|V n |<2 % of V out <10 %

32. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 32 Drivers status Parameters to improve (2) PARAMETERREF.SPEC. ACHIEVED Propagation delay time T D dependent on T Wout T D dep. on rep. freq. TDTD <500 ns No <100 ns No Yes: ≤0.2ns @ 1MHz ≤1.5ns @ 15MHz Pulse dist. | T Wout - T Win | T Pd dep. on T Wout T Pd freq. Pd<5 ns No <3 ns Yes Yes: ≤0.2ns @ 1MHz ≤1.2ns @ 15MHz

33. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 33 Drivers status Synchronization electronics Fast synchronization electronics prototype has been developed. It is composed of : a synchronism detector. a fast adjustable delay. digital pulse to pulse loop that locks the rising front of the amplifier output pulse to a reference pulse. This compensates slow delay variations (max 30 ps/pulse) and stabilizes the delay within ~100 ps. A similar loop can also be built to compensate the delay variations.

34. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 34 … finally   The achievement of the full specifications seems to be a very complicated task and the experience gained until now is very important.   The rise and fall time are only part of the difficulties as pulse delay and pulse length distortion are also very difficult to be maintained within a fraction of ns.   Even if only partially fulfilling the specifications, 3 units of each polarity will be delivered at the end of November 2008. They will already implement some improvements.   The availability of the drivers will allow testing in 2009 the overall chopper system without beam.   The development will then continue to achieve full specs.

35. Caspers,Paoluzzi CERN chopper status October 2008 CERN HIPPI meeting October 2008 35 Acknowledgements   We would like to thank the AB-RF workshops for assembling the tank, F. Wurster, M. Nagata and Mr U.Behrens from Kyocera for fruitful cooperation in development and implementation of the technologies for printing the meander structure   J. Borburgh for assistance with the heat transfer measurements and in particular Vladimir Bretin and his crew from the RF mechanical workshop for his infinite patience and diligence in mounting and demounting this structure.   Thanks also to R. Garoby and T. Linnecar for support

36. How to integrate the CERN chopper concept into ESS F. Caspers Due to the high peak power (80 kW = 2kV on 50 Ohm) required when using a COPYPASTE of the CERN version, I would expect huge problems there in particular for the driver (pulser)..and not recommend this. But we don’t need 2..3ns rise and fall time for ESS anyway. If we are allowed to use electronic components near the chopper tank (e.g. fast Schottky power diodes, maybe some rad hard version and or some shielding) we could apply a kind of macroscopic “sample and hold “ circuit there and just have a normal metallic plate for deflection. In this case we would have a short “charging” pulse on one cable and another “discharge” pulse on another cable (together with the diodes)..and no meander line Another option may be some active load circuit, since in principle we just require a short yet powerful “charge/discharge” pulse..and we have to avoid reflections on long pulse transmission lines..leading to fake pulses seen by the beam.