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Europe/Zurich
6/R-012 - conference room (CERN)

6/R-012 - conference room

CERN

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Correction debugging, Tobias

Corrections of chromatic coupling did not work surely due to not using output files _free, which remove the effect of AC dipole. 

ACTION -> Tobias & Jaime investigate and fix by next Thursday since Jaime leaves.

(Meghan, Andy, Jaime and Tobias leave Thursday or Friday)

 

Optics corrections probably worked but the python getdiff script was not using new results. -> Tobias & Jaime to look at it.

MQT effect -> Andy

MQT update button enough? need input time?

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IR8 insigth, Lukas

IR8 corrections only measured for Beam1. 

Q1L8 -3.3e-4

Q1R8 +4.5e-5

horizontal plane looks very noisy before and after correction. While Vertical plane really matches

expectations even with the sign as trimmed in the machine.

Since horizontal data does not allow to determine if horizontal correction worked maybe it was wise

to remove correction.

ACTION -> Re-analyze: (1) before and after correction with only 1000-2000 turns so BPMs are removed and using latest syst. errors from Andy -> Lukas and Andy (Jaime already changed the large p2p cut of 20mm)

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Model masks, Jaime

To avoid too many templates some MADX macro library is being setup that is joined via python. We must avoid repetition.

Interesting and powerful.

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dipole systematic b2 effect, Andy

For beam 1 the dipole quadrupole error is enough to explain the difference between 6.5 and 4 TeV.

For beam 2 it is not so clear. Maybe some discrepancy comes from teh fact that models are different in 2012

and 2015.

ACTION-> check the impact of different models

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Beta from amplitude, Ana

Bad calibrated BPMs identified (mostly BPMS, skew). 

3-4% rms in the difference between from-amp and from-phase

ACTION-> systematic analysis to compare to newer data.

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PSB, Meghan -> interesting results and lots of measurements for next week.

It is known that BPMs not working is due to some head amplifiers missing. These will be installed

in August. They have a guess for the 136 kHz signal.

ACTION-> Ana starts looking into PSB and we have a meeting.

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non-linear correction, Ewen

Corrs worked but MCO was a bit large, about 10%, and MCD was a bit low.

Source could be orbit or hysteresis, to be checked.

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AOB - Best knowledge model

Lukas can look at impact on global corrections in beta measurements

and then we see how to stablish a best knowledge model.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

There are minutes attached to this event. Show them.
    • 16:00 16:10
      Chromatic coupling and corrections 10m
      Speaker: Tobias Hakan Bjorn Persson (CERN)
    • 16:10 16:20
      IR8 insight 10m
      Speaker: Lukas Malina (Charles University (CZ))
      Slides
    • 16:20 16:30
      Model masks 10m
      Speaker: Jaime Maria Coello De Portugal - Martinez Vazquez (Ministere des affaires etrangeres et europeennes (FR))
      Slides
    • 16:30 16:40
      dipole b2 10m
      Speaker: Andy Sven Langner (Hamburg University (DE))
      Slides
    • 16:40 16:50
      beta from amplitude 10m
      Speaker: Ana Garcia-Tabares Valdivieso (Ministere des affaires etrangeres et europeennes (FR))
      Slides