activities in mainz
DESCRIPTION
Activities in Mainz. David Lomidze, Andreas Winhart Universit ät Mainz. MUV working group meeting CERN 15 Dec 2010. Investigation of properties of Protvino scintillator using: Cosmics Laser Radioactive Source LED system Automatic test line for mass-test Setup for Prospective PMT test. - PowerPoint PPT PresentationTRANSCRIPT
MUV WG meeting. CERN 15.12.2010
Activities in Mainz
David Lomidze, Andreas Winhart
Universität Mainz
MUV working group meetingCERN 15 Dec 2010
MUV WG meeting. CERN 15.12.2010
Outline
• Investigation of properties of Protvino scintillator using:– Cosmics– Laser– Radioactive Source– LED system
• Automatic test line for mass-test • Setup for Prospective PMT test
MUV WG meeting. CERN 15.12.2010
Laser setup
Advantage: well defined pulses, fluctuations canceled by energy diode
Disadvantages: Low rate (10Hz), Scintillator must be unwrapped
PM_L PM_R
Ultraviolet Nitrogen Laser
Wavelength 337 nm
Mimics p-Terphenyl
UV Laser Generator
Light distributor
Nitrogen Source
Trigger diode
Filter
Energy diode
Reflector
MUV WG meeting. CERN 15.12.2010
Setup for PMT photo window uniformity
x
y
~20% fluctuation expected
MUV WG meeting. CERN 15.12.2010
PM surface scan
~20% fluctuation of PMT photo window as expected
MUV WG meeting. CERN 15.12.2010
Sr90 Setup
A&B – Read out PMTs
T1&T2 – Trigger PMT
St – Trigger Scintillator, 0.5mm Thickβ energy end point
0.5 / 2.3 MeV
A B
T1 T2
Sr90
St
Collimator
Advantages: High rate ~1KHz (High speed for testing)
Disadvantages: Difficult for energy calibration, Wide range of energy, because of β spectrum nature
MUV WG meeting. CERN 15.12.2010
Sr90 SpectrumTypical Beta energy distribution
Mean value and area under curve can be used as relative estimators for strip quality
Measured beta spectrum, from two different PMT
Full spectrum of Sr90
Theoretical
Experimental
MUV WG meeting. CERN 15.12.2010
Sr90 Collimator (Electron Spectrometer)
FieldSN
CurrentForce
Sr90
First Collimating hole
Hole for Magnet
Second Collimating hole
+ -
NS
Magnet
Threshold
At this moment this is at just an idea, but we will try to realize it!
MUV WG meeting. CERN 15.12.2010
LED system
Several LED with different wavelengths
• 270 μm – to activate p-Terphenyl
• 337 μm to mimic Laser
• 490 μm to mimic WLS fiber light (for mass test of PMTs)
Work in progress on ultrafast LED driver:
1.5ns pulse rise/fall time
Variable pulse length (6ns – 200ns)
Variable pulse size (few mV to 10V)
Variable rate from few Hz up to 100 MHz (for PMT)
MUV WG meeting. CERN 15.12.2010
LED system
There are few ways for long scintillator tests with LEDs:
Put several LEDs under scintillator (Very fast but expensive way (~170€ each LED))
Drive light from one LED with bundle of clear fibers
Move one LED along scintillator by stepping motor (Bit slow, but low cost way)
MUV WG meeting. CERN 15.12.2010
Automatic line for mass-test
Cosmics Trigger
Laser
MUV WG meeting. CERN 15.12.2010
Intermediate box for merging Windows and Linux applications
Why needed it?1. Stepping motor controller application needs windows platform and DAQ is
running under Linux SLC4• But… IT650Flash controller has 4 bit input port, which can be used for CAMAC TTL
signals to control it
2. Extremely high noise - when motor is powered– Few power supply filters have been tried unsuccessfully to solve it
– No noise if motor is disconnected from controller
Way out – intermediate box
24V relies – to disconnect motor before data taking till next movement
Auto operation mode
RS232 serial connector for automatic control by CAMAC – to generate 4 bit signals + one control line to activate/deactivate relies
Manual operation mode
MUV WG meeting. CERN 15.12.2010
New Mask
• While testing of several samples – observed, that coupling can influence measured Nphe– Main problem -> sometimes not having same length of free
fibers after gluing on each side of scintillator sample (~1/2 mm)
• To exclude geometrical fluctuations:– New PMT mask with holder have been designed
Features:
1. Always 90o angle between WLS fiber and PMT Photo Window (PPW)
2. Keeping end of fibers always at same distance from PPW
3. Variable distance between fibers ends and PPW
MUV WG meeting. CERN 15.12.2010
Measurement with Laser
X10 cm
Npe
# of Photo Electrons VS Scintillator length
Lowest signals from central region ~8.3 Photo electrons from single PM
But ~16phe from sub-channel and 12x16=192phe longitudinal channel
1900 x 40 x 10 mm3 scintillator sample with two glued fibers
MUV WG meeting. CERN 15.12.2010
Study of relative light output in WLS fibers using laser
400 x 40 x 10 mm3 Scintillator sample
•One end read-out by 5mm thick plexiglas
•Other end by two WLS fibers, glued along strip
90 x 2 = 180 Phe = total Blue light
12 Phe in two WLS fibers, Green light
~6.6% of light in two WLS fibers
MUV WG meeting. CERN 15.12.2010
Study of relative light output in WLS fibers using laser
90 x 2 = 180 Phe = total Blue light
12 Phe in two WLS fibers, Green light
~6.6% of light in two WLS fibers
(Fiber trapping Efficiency (5-6%)
&
PMT Quantum efficiency plays significant role)
Quantum efficiency ~16% (at 500nm) (~28% at 390nm)
MUV WG meeting. CERN 15.12.2010
Wrapping test
Wrapped
Unwrapped
Light output doubled!
MUV WG meeting. CERN 15.12.2010
Summary table of cosmic test of WLS fibers
Npe
Fiber type Nr of Fibers R2076 R1924A R6095
Bicron 1.2mm MC Round 3 5.3 16 14
Bicron 1.2mm MC Round 2 8 16 6 11.3 6.5 14
Bicron 1.0mm MC Round 2 4 9 3.5 7.2 3.5 7.5
Kuraray 1.0mm MC Round 2 10 21 8.4 17.6 9.5 19.3
Bicron 1.2mm MC Square 2 4 8.2 3.8 7.7 4 8
Bicron 1.2mm MC Round 1 8.9 7.6 9.12
Bicron 1.0mm MC Round 1 5 6 5.4
Kuraray 1.0mm MC Round 1 10.5 10.5 11.9
Bicron 1.2mm MC Square 1 5 6.3 6.1
Bicron 1.2mm SC Round 1 6.5 5.2 6.6
Bicron 1.2mm MC R (BCF-91A) 1 7.6 6.3 8.9
Bicron 1.2mm MC Round 2 11.2 9.1 10.1 NOT Glued 1.5X1.7mm^3groveBicron 1.2mm MC Round 2 17.6 13.8 15.4 Glued
Bicron 1.2mm MC Round 2 10.7 8.3 9 NOT Glued 1.3X1.5mm^3groveBicron 1.2mm MC Round 2 11.3 8.8 Glued
- Npe from single fiber
- Npe from all fibers
MUV WG meeting. CERN 15.12.2010
MUV1 single channel design
• Considered fibers for single channel construction:– Single Kuraray or Two Bicron 1.2mm round MC fibers
• 2XBicron delivers ~40% more light than single Kuraray fiber• two fibers are more safe
• Wrapping – significant improvement for light collection
• Gluing gives ~50% more Photo electrons• Groove size for 1.2mm fiber – 1.5 x 1.6 mm^2• Number of Grooves = 2
MUV WG meeting. CERN 15.12.2010
Outlook
• Test setup for 1000 scintillator test: Ready with laser Ready with Sr90 full spectrum– Laser alternative way – LEDs getting ready
• LED driver – experts are involved, already have a prototype– Put threshold on Sr90 spectrum –work in progress (designed first
prototype, needs modifications)• MUV1 PMTs test:
Laser system ready!– LED system in way of development
• MUV2 PMTs– HAC PMTs recently moved to Mainz, quality test will start after
New Year
• Scintillators with final dimensions needed asap!– additionally we NEED to have low quality scintillators
(bubbles, dust, low or high fraction of scintillation material) to check quality/efficiency of our system