ondřej svoboda for the ecal group hades collaboration meeting xxv, 19 – 23 november 2012 gsi
TRANSCRIPT
Tests of ECAL modules with LED induced light and cosmics
Ondřej Svoboda for the ECAL group
HADES collaboration meeting XXV, 19 – 23 November 2012 GSI
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Summary of ECAL test setup development since last
collaboration meeting:
- continuous delivery of new 3 inch photomultipliers
(Hamamatsu R6091)
- new mounting construction designed, manufactured and tested
- prototype of HV divider for R6091 photomultipliers
constructed and tested
- one module with optical fiber and LED diode assembled and
successfully tested (8/2012)
- based on this 5 modules with 1.5 inch EMI 9903KB
photomultipliers and 5 modules with 3 inch R6091
photomultipliers assembled, all with optical fiber
- light guide system to drive all 10 modules with one diode
assembled
- tests of new TRB based Front-End – see talk of Behruz Kardan
- first test of 3 inch photomultipliers – Yuri Sobolev
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Layout of HV divider for 3 inch photomultipliers (Hamamatsu R6091)
- Reason for development and manufacture of own HV divider is the price of original ones…
- First tests show that the divider is comparable with the original Hamamatsu divider (same current, comparable pulse shape and amplitude from the detector).
- To confirm this further tests are needed and will be done in close future.
Produced by CPM Jičín, CZ
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New housing for R6091 3 inch photomultipliers
Magnetic shielding produced in IP Bratislava
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Cosmics measurement
3 inch photomultiplier (Hamamatsu R6091)
1.5 inch photomultiplier (EMI 9903KB)
Energy resolution: 5.9% (best case up to now)
Energy resolution: 5.4 % (best case)
ADC (channels)
For measurement used CAMDA system and shaper MA8000
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Tests of diodes for stability monitoring of the ECAL modules
Continuous search for optimal solution from many possibilities:
- one diode per module, coupled to lead glass via optical Si fiber (20 cm)
- different light output from each diode (+-50%)
- one diode per sector, light guides to each module- how to distribute the light homogenously to each module?- which fibers, connectors will be used (question of price)?- light source to “power” all sector
- common diode will be most probably weak- high power diode needs higher voltage and current – hard for 10 ns pulses- laser sources – up to now tested one for single mode fibers
- red light (not ideal for photomultiplier) - slow (not able to produce 10 ns pulse of the
same amplitude)- very expensive
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Layout of the ECAL testing setup with LED
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Light guide system for 10 modules
Diode with light distribution system and 10 fibers
Light output from diode
Fiber to lead glass transition
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Measurement with LED diode
- very fast measurement (kHz) in comparison with cosmics (~1 signal /3 minutes)- signal from pulser set to get the same detector response as from cosmics
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(Ham
am
ats
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R6091
)
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oto
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fter
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oard
Yellow curve – detector outputGreen curve – diode input (second peak is reflection
on diode)
10Measurements made by Y. Sobolev on CAMDA system
Measurement with LED diode and 3 inch photomultiplier Hamamatsu R6091
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Summary:
- LED can be used for regular stability monitoring of ECAL during beamtime
- basic assembly of ECAL module driven by LED diode successfully tested
- search for final LED system design
- new housing for R6091 3 inch detectors
- first tests of own HV dividers for R6091 3 inch photomultipliers
- tests of ECAL modules with both types of PMT‘s on cosmics and with LED diode performed
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Thank you for your attention…