MD#2 News & Plan Tue – Wed (19. – 20.6.)

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Presentation transcript:

MD#2 News & Plan Tue – Wed (19. – 20.6.) Day Time MD EiC MP Tue 06:00 450 GeV  4 TeV: Ramp for chromaticity (done later) A 08:00 Ramp down 10:00 450 GeV: Large Piwinski Angle MD + precycle 2 bunches 2.4e11 – started with 3:30 h delay 18:00 450 GeV  4 TeV: Octupole instability threshold Single full physics beams – successful Ramp for chromaticity + octupole effect C Wed 02:00 04:00 450 GeV  4 TeV: Longitudinal dynamics studies– successful B 12:00 450 GeV  4 TeV: Beta* leveling 2 nominal bunches – successful 20:00 22:00 450 GeV  4 TeV: Long-range beam-beam with high bunch intensity 84b 50 ns 1.7e11 – successful Giulia Alick Ghislain Giulia Mirko Alick Ghislain 22-06-12 MD#2 News & Plan 22 June 2012

Draft MD Planning Thu – Fri (21. – 22.6.) Day Time MD EiC MP Thu 06:00 Ramp down 08:00 450 GeV  4 TeV: High beta* (1) – successful A 16:00 18:00 450 GeV: MKI UFO studies C Fri 04:00 450 GeV  4 TeV: Scraping, diffusion and Repopulation Study and fast losses (with ADT) C+C 12:00 14:00 450 GeV: Injection and Q20 optics 22:00 450 GeV: RF cavity phase modulation for 25ns B Ghislain Mirko Alick Ghislain Verena Mirko 22-06-12 MD#2 News & Plan 22 June 2012

Draft MD Planning Sat – Mon (23. – 25.6.) Day Time MD EiC MP Sat 06:00 450 GeV  4 TeV: High beta* (2) A 14:00 Ramp down 16:00 450 GeV: Transverse Damper studies - cancelled 22:00 Sun 00:00 450 GeV  4 TeV: Collimation (impedance, nominal settings) C 08:00 450 GeV: Beam Instrumentation (BSRT, BGI, wire scan, BPM nonlinearities) A/B/C 450 GeV  4 TeV: Test ramp for emittance calibration B/C 20:00 450 GeV: Dynamic Aperture MD D Mon Technical Stop Alick Enrico Mirko Alick Enrico Mirko Alick 22-06-12 MD#2 News & Plan 22 June 2012

High beta* (1) Aim: beta* = 500 m in IP1&5; measure & correct optics 3 probe bunches per beam, initial intensity ~3e10 per beam First 3 hours: re-commissioning of the 90 m optics with parallel separation on, Q’ measured and corrected in several steps to 90 m Collimators opened up at 90 m for the de-squeeze The de-squeeze from 90 to 500 m worked very well without any significant losses. The second half of MD: optics measurements and corrections at 500 m. AC dipole beam 1 horizontal plane faulty and requires access to reset. Measured optics B1 V and B2 H/V. Beta-beat without correction mostly within +/- 20 %. Corrections were calculated online and implemented and optics quickly re-measured. H. Burkhardt, J. Wenninger, M. Pojer, M. Solfaroli, S, Redaelli, L. Ponce, beta-measurement team et al.

Optics Measurements at 500 m Beam1 The AC dipole malfunctioned in the H-plane of Beam1. A global correction for beam1 was calculated using data from the 90 m commissioning on Monday night where some initial measurements at 500 m had been made. Optics was re-measured with the global correction implemented, kicking only in the V-plane with the AC dipole. There is no usable data for the B1 H-plane from the MD Beam2 Optics measurements were performed on and off momentum with no correction applied. Local corrections were calculated for IP1, IP5 and IP6. Optics was re-measured on-momentum with local corrections implemented. A global correction was calculated on the phase. Optics was re-measured with local and global corrections implemented.

Optics Measurements at 500 m

MKI UFO studies T. Baer, M. Barnes, R. Giachino, G. Roy access for BLM diamond sensors at Pt7, and for B1 MKQA (successfully repaired and tested by the piquet); started real MD at about 20:00 test procedure for non-standard MKI operation ~1.15 hours PS cavity problem & beam losses when injecting 144 bunches with large emittance (beam dump), solved by TL steering at ~0:50,1236 bunches were circulating for B1 and B2 with two different emittances of ~3, ~1.5 mrad (blow up by screens) pulsed MKIs in gap alternating for B1 & B2 to produce UFOs; at 1:40 h switched off MKI e-cloud solenoids - 10 min later flashover at MKI.C5R8 with vacuum interlock ventilation door opening in Pt.2, ended the MD MKIs pulsed 48 times; several UFO events observed 1 conclusion: don’t operate MKIs without e-cloud solenoids

MKI UFO studies - emittances

UFO event about 30 ms after MKI pulse

loss spikes after MKI pulse

Scraping, diffusion & repopulation study F. Burkart, G. Valentino, S. Redaelli et al ++ scraping & collimator retraction at top energy in squeeze w/o collision with collision Asynchronous dump test next: ADT fast losses