1um pilot prepared | In preparation | |
Dedicated LHC cycle | If problems with present supercycle |
Magnets | Required circuits here | ||
Power Converters | Should be fully tested out following hand over of sector to operations. 450 GeV and pre-cycling. Mike's list here Sector 34 and 45 mains condamn and will remain so. |
Mike/Lasse/Delphine | |
Injection System | Brennan's list here | Brennan | |
Septa | FCCM | ||
Septa | Trim Strengths | ||
Septa | Check calibration curve | Jorg OK | |
RF | Rephasing & synchronization between SPS & LHC must be established. So far SPS re-phasing not with LHC RF frequency. Requires exchanging the existing pre-pulse generation system with a new ‘LHC style’ system – will affect all SPS beams (also CNGS). To be done second half of July. |
Andy | Test Mon 28th |
TDI | Very basic functinality required - essentially in/out | Stefano | OK |
Collimators | Configuration at IR3 - strategy to be confirmed. | Stefano/Helmut/Mike |
|
Alice |
|
||
Vacuum |
|
Gianluigi | Situation at point 3? Do we need 34 < 5 K |
System | Requirements | Issues | |
---|---|---|---|
BLMs | Mobile BLMs? Difficult apparently - won't have any extra before. Even going in during test if necessary could be problematic | Bernd/Lars |
|
BLM BLM requirements | Will 23 have been tested with source? | ||
BLM | Connect to BIS and test. | Bruno/Markus/Rudiger | |
BPMs |
|
Marek M. |
|
BTVs |
|
||
BCT - end TI2 | Standard | Markus Albert | |
RADMON | Gateways covering Q5.L2 to IP3.R available week 30 (cfc-sr-sl2a, cfc-sr2-sr2b, cfc-sr3-st3a) c/0 Anna Nyul | ||
RAMSES | Check |
|
|
BIC | What's the issue with logging? | ||
Full list here
System | Main Objectives | Comments | |
---|---|---|---|
Extend TI2 | Put in TI2 respository and LSA | Massimo | Done |
Optics | V6.503 - need also TI2/LHC continium | Done | |
Optics | Use Old or re-match TI2 optics? Decision required. | ||
FIDEL |
[requirements] | FIDEL will provide coefficients for all circuits involved. | |
Aperture model | Extend from MSI to TDI | Bren | Done |
On-line model | What are our use cases? | ||
MCBYV.B4L2.B1, MCBYV.A4L2.B1 and MCBYV.4R2.B1 and MCBYV.5L2.B1 | |||
Nevertheless from the oscillation and QT data I have a few preliminary findings: - QTL11R2 appears to be inverted - polarity of QT12R2 looks OK - data taken for QT13R2 are too noisy to conclude on its polarity; I hope to get information on this by playing with the model and comparing with better oscillation data - BPM.33R2.B1 probably has the wrong polarity - as you know there is another (larger) optics error between Q17L3 and Q7L3; in x it is almost explained by an inversion of Q7L3 (but this is not it!); it is big, inversion of Q7L3 could explain the x data but not the vertical ones, an inversion of QTL11L3 cannot be the source of this optics error; - MQS has no effect; perhaps not connected? (or did we not trim it correctly??) - x and y phase advances in the arcs seem to deviate from my model; x oscillation propagates a little faster and y a little slower than I expected |