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BPM for Spectromety development status A. Lyapin.

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Presentation on theme: "BPM for Spectromety development status A. Lyapin."— Presentation transcript:

1 BPM for Spectromety development status A. Lyapin

2 WP 4.2 meeting, 13 September 20062 Summary  BPM design more or less finalized  Al prototype ≥50% done, need ~2 weeks  Need to test the model and fix the tolerances ~2 weeks, may need to modify the design – got nicer feedthroughs  Test bench is operational  Cu (vacuum) prototype – design ≥50% done  Planning to start cutting copper in October  Material (OFC) purchased  Reference cavity – just started with the electrical design so far  Signal processing electronics – overall layout finalized, looking for components, putting together spreadsheets  Calibration scheme – overall layout finalized, key components found, quotes received (~£2-3k project)

3 WP 4.2 meeting, 13 September 20063 Prototype Al model  MSSL finished working on the waveguides (spark erosion)  UCL workshop to continue this week  Slots, holes for the feedthroughs to be put in, beam pipe to be cut to the dimension, other bits and pieces to be put in

4 WP 4.2 meeting, 13 September 20064 Prototype Al model

5 WP 4.2 meeting, 13 September 20065 Cavity BPM test bench  Test bench is up and running  2.8 GHz oscillator is on its way to UCL  VNA is on its way to RHUL

6 WP 4.2 meeting, 13 September 20066 Cu vacuum prototype  Most of the problems cleared, brazing seems to be ok  DN63 flanges to fit the rest of the ESA beamline, 8 through holes for support  Need to modify the feedthroughs  Reduced the length for easier machining, monopole rejection should be sufficient  Need some input from KEK on tuners

7 WP 4.2 meeting, 13 September 20067 Reference cavity

8 WP 4.2 meeting, 13 September 20068 Electronics

9 9 Electronics

10 10 Electronics

11 WP 4.2 meeting, 13 September 200611 Calibration scheme  Probably a final scheme now  Can actually use the drive line power, but want to use it for the LO  Still need to find suitable (high conversion gain) detectors  Passive elements are not a problem

12 WP 4.2 meeting, 13 September 200612 Calibration scheme


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