TOF Status Report TIM at CERN, Geneva, 27 Oct' 1 Nov' 2003 F'Palmonari, INFN - PowerPoint PPT Presentation

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TOF Status Report TIM at CERN, Geneva, 27 Oct' 1 Nov' 2003 F'Palmonari, INFN

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Title: TOF Status Report TIM at CERN, Geneva, 27 Oct' 1 Nov' 2003 F'Palmonari, INFN


1
TOF Status ReportTIM at CERN, Geneva, 27 Oct.
1 Nov. 2003F.Palmonari, INFN University of
Bologna
  • Summary
  • Overview
  • Mechanics
  • Electronics

2
Overview of work done since last TIM
  • Tenders for TOF planes mechanics started
  • Much work to optimize the design of TOF-ACC
    electronics to save weight and cure thermal
    issues
  • Preparation of the Test run on the Ion beam

3
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4
G.F. 5000 cm2 sr Exposure gt 3 yrs
dP/P2 0.004 ? MDR 2.5 TV, h/e 10-6 (ECAL
TRD)
5
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6
The TOF Scintillation Counters
  • 4 planes of plastic scintillation counters slabs
    1 cm thick
  • 8( X ) 8( Y ) counters Upper TOF above Magnet
  • 10( Y ) 8( X ) counters Lower TOF below Magnet
  • 34 counters seen at both ends by a pair of R5946
    Hamamatsu PM
  • 144 PMs in total, giving Anode and 3rd-last
    Dynode signals
  • 68 HV channels
  • 68 Anodes 68 (144 tbd) Dynodes signals

7
AMS II TOF Mechanics
FEM model finished (with USS displacement) The
goal is to mount the complete Lower TOF Spring
2004 to perform a vibration test to check The
adopted design solutions PMTs fixation, Light
guides bending, internal cabling
8
AMS II TOF Mechanics
9
AMS II TOF Mechanics
Lower TOF
10
AMS II TOF Mechanics
11
Overview on electronics
  • Most progresses concern the electronics Hardware
    of the TOF system
  • Both LV and HV Power supplies have been
    simplified to gain weight
  • The TOF-ACC scintillator crate SCR has also been
    redesigned
  • The Dynode ADCs have been moved on the detector
    to simplify cabling and save weight
  • See Guido Castellini report on Thursday

12
The previous Scintillator Crate
13
The 1500-2300 V HV regulator channel.Paking is
optimized for complete potting.
14
The previous S-Crate modules
15
Test run preparation in Bologna
  • The team of young people (Diego and Beppe are
    old). From left Lorenzo Villa, Lucio Quadrani,
    Roberto Martelli, Veronica Bindi, Dafne
    Baldassari, Cristina Sbarra, Fernando Massera,
    Luca Amati. (Francesca Giovacchini and Alberto
    Oliva are not there)

16
Purposes of the test run
  • Take relativistic Ion data on 4 counters like in
    AMS-02 to study
  • 1)overall resolution in Z
  • 2)multiple hit, fragmentation in plastic
    scintillator
  • 3)saturation effects
  • We use counters with different light-guides
  • Two straight light-guides as in planes 1 and 4
  • One bended (counter 302)
  • One bended and twisted (counter 205 )
  • Test the EM front-end cards SFET and SFEC, mainly
    for thresholds and ADC dynamic range setting

17
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18
TOF Planes Assembly Plan
  • Phase 1 - PMs assembly started mid February
    ENDED.
  • Phase 2 - PMs calibrations started in March,
    ENDED 192 PM done (144 will be mounted
  • Phase 3 - The flight scintillation counter slabs
    machined and ready for light-guides glueing have
    been delivered. Glueing and wrapping
    started in September
  • Phase 4 - Scintillation counters
    characterisation.
  • Phase 5 - Counters assembly with PMs, vacuum test
    and calibration with cosmic rays will start in
    January with Lower TOF.

19
Study of the optimisation of the PM disposition
to take into account that we have to power them
in pairs to save weight and power.
  • Each of 245 PMs ( in a relational database) is
    characterized by many quantities
  • Gain as function of HV
  • Gain derivative at the setting HV
  • Photocatode luminous sensitivity
  • Dark current, etc..
  • When mounted the PM response depends also on at
    least two other quantities
  • The trasmission coefficient of his lightguide
  • The gain change due to the magnetic field in his
    position
  • To take into account all effects when two PMs are
    powered together and find the best way to choose
    144 PMs out of the 200 we have is not simple.
  • An optimisation program using a genetic algorithm
    has been developed.

20
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21
Counters characterisation is made inside a
light-tight box.Infact they are prepared with
the aluminized mylar wrapping alone.
22
Preparation of the BENT and TWIST LG CountersPM
chosen from optimisation table
23
Results of the characterisation on the Cosmic Ray
Telescope
24
The new SFET on the test bench
25
The ADC card using the RICH Chip under test
26
Conclusions
  • The TOF counters preparation is going on within
    schedule
  • The counters calibration will help in the final
    setting of all parameters of the front end
    electronics
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