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Synchrotron Radiation Detector Studies

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Presentation on theme: "Synchrotron Radiation Detector Studies"— Presentation transcript:

1 Synchrotron Radiation Detector Studies
ETH-ZURICH Volker Commichau, Hanspeter von Gunten Hans Hofer, Ulf Roeser, Gert M. Viertel KNU Manwoo Lee EWHA Kyung Sook Kim SRD / PEBS/ January 2009 / GV / ETH

2 S. A. Stephens, V. K. Balasubrahmanyan, Earth’s magnetic field as a radiator to detect
cosmic ray electrons of energy > 1012 eV, J. Geophys. Res. 88, A10,7811 (1983) 1998 SRD / PEBS/ January 2009 / GV / ETH 3

3 2005 SRD / PEBS/ January 2009 / GV / ETH

4 ~ m Trigger Device SRD / PEBS/ January 2009 / GV / ETH

5 SRD / PEBS/ January 2009 / GV / ETH

6 SRD / PEBS/ January 2009 / GV / ETH

7 SRD / PEBS/ January 2009 / GV / ETH

8 SRD / PEBS/ January 2009 / GV / ETH

9 Number of synchrotron photons on the
SRD for an electron energy of 10 TeV for various SRD detection ranges x SRD Model Magnetic Field: 400 mG ½ l: 1.6 m SRD / PEBS/ January 2009 / GV / ETH

10 Energy distribution of synchrotron photons
for various detection ranges of the SRD SRD / PEBS/ January 2009 / GV / ETH

11 Technical Publication: H. Anderhub et al., NIM A491 (2002) 98-112
SRD / PEBS/ January 2009 / GV / ETH

12 PSRD : X-Ray Detector SRD / PEBS/ January 2009 / GV / ETH 3

13 Small YAP SRD / PEBS/ January 2009 / GV / ETH

14 Large YAP Crystal Assembly
Veto PMT Output & Bias (5 mm Plastic Scintillator) PMT Output & Bias 30 x 30 x 30 mm3 YAP SRD / PEBS/ January 2009 / GV / ETH

15 Large YAP Tor-Lm (“Mylar”) Window 5 mm NE102A 30x30x30 mm3 YAP
SRD / PEBS/ January 2009 / GV / ETH

16 Macro Strip Detector With APV Readout
SRD / PEBS/ January 2009 / GV / ETH

17 SRD / PEBS/ January 2009 / GV / ETH

18 Typical event 8 bit ADC 50 ns / channel
SRD / PEBS/ January 2009 / GV / ETH

19 YAP: 18x18x1 mm3 YAP: 30x30x30 mm3 [AU] MET [h] Counts/sec Counts/sec
South Atlantic Anomaly [AU] MET [h] Averaged Gate Content: (# of Signals per Gate) / 10: Latitude: PMT Current: PSRD Attitude: Deep Space SCA >10 keV Channel: SCA >40 keV Channel: SCA >120 keV Channel: YAP: 30x30x30 mm3 SCA Charged Particle Channel: Solar Cell : LED Test Pulse Counts/sec Counts/sec South Polar Region North Polar Region MET [h] H. Anderhub / ETHZ SRD / PEBS/ January 2009 / GV / ETH

20 PSRD Attitude: Deep Space YAP # 4B
YAP (18 x 18 x 1 mm3 / 50 μm Be Window) SAA & Pole Regions excluded SAA and Pole Regions No Sun Sun No Sun Sun B. Zimmermann / ETHZ SRD / PEBS/ January 2009 / GV / ETH

21 MIP Small YAP PSRD Attitude: Deep Space No Sun SAA & Poles excluded
Direct Channel Attenuated Channel (x10) MIP B. Zimmermann / ETH SRD / PEBS/ January 2009 / GV / ETH

22 PSRD in the Polar Region
Small YAP 1A Small YAP 6A ~ 100 keV ~ 140 μsec SRD / PEBS/ January 2009 / GV / ETH

23 PSRD (Small YAP): All Attitudes, No Direct Sun
North Pole Counts / (Small Yap[4B] x sec) Solar Flares South Atlantic Anomaly South Pole B. Zimmermann / ETHZ SRD / PEBS/ January 2009 / GV / ETH

24 Results from the PSRD Mission
Measurement of the background: Outside the polar regions, the South Atlantic Anomaly and during years of moderate/low sun activities: The SRD concept can be realized . Usefulness of the APV readout for space application proven (Time resolution < 10 ns & high readout density). Detector components: Space qualified. SRD / PEBS/ January 2009 / GV / ETH

25 GSO: Gd2(SiO4)O-Ce YAP: YAlO3-Ce YSO: Y2(SiO4)O-Ce BGO: Bi4Ge3O12
SRD / PEBS/ January 2009 / GV / ETH

26 SRD / PEBS/ January 2009 / GV / ETH

27 Cerium doped Yttrium Perovskite [YAP(Ce)]
SRD / PEBS/ January 2009 / GV / ETH

28 HAMAMATSU R5900U SRD / PEBS/ January 2009 / GV / ETH

29 ~50 % SRD / PEBS/ January 2009 / GV / ETH

30 SRD – TRD Concept 1.2 m x 1.2 m TRD 1600 Cells
SRD / PEBS/ January 2009 / GV / ETH

31 SRD / PEBS/ January 2009 / GV / ETH

32 SRD / PEBS/ January 2009 / GV / ETH

33 TRD – X-tal Test at CERN SRD / PEBS/ January 2009 / GV / ETH

34 TRD – X-tal Test Results (Sample)
SRD / PEBS/ January 2009 / GV / ETH

35 Single Cell Crystal YAP/Other Crystal 30x30x30 mm3 PMT/Other Hamamatsu
Subsegment 64 Cells PreAmp Bias TorLM Window not shown (Light Shield) SRD / PEBS/ January 2009 / GV / ETH

36 SRD / PEBS/ January 2009 / GV / ETH

37 Time resolution measurement with Mn54 source
SRD / PEBS/ January 2009 / GV / ETH

38 SRD / PEBS/ January 2009 / GV / ETH

39 SRD / PEBS/ January 2009 / GV / ETH

40 PMT ~ 0.05 W (Preamp) + 0.02 W (Bias) 1600 x 0.07 W
SRD-TRD Design Study: Power Consumption PMT ~ 0.05 W (Preamp) W (Bias) 1600 x 0.07 W APV ~ 0.3 W x 0.3 W ADC + RAM +I/O ~ 0.3 W 25 x 0.3 W TDC + programmable Delay ~ 0.2 W 25 x 0.2 W PLD + I/O ~ 1.0 W x 1.0 W TRD x 0.07 W Computing W Slow Control 2 W Data Storage 5 W Total Power (Estimated) : W Weight (Estimated) kg SRD / PEBS/ January 2009 / GV / ETH

41 Conclusion The Synchrotron Radiation Detector can be built and operated except for the polar regions and SAA, excluding also direct sun. This device can measure the sign and energy of multi-TeV electrons and positrons in a high hadron background. The SRD – TRD design concept including fast scintillators with high light yield for both sub-components (TRD & SRD) has advantages: Excellent time resolution Low power consumption Low weight High efficiency Low background from trigger device back splash Simplified TRD operation (No gas system) SRD / PEBS/ January 2009 / GV / ETH


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