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M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

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Characterization of triple-GEM detectors constructed with a low-cost stretching technique using infrared heating. M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann Department of Physics and Space Sciences Florida Institute of Technology. Presentation Outline. Outline GEM Design - PowerPoint PPT Presentation
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M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann Department of Physics and Space Sciences Florida Institute of Technology
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Page 1: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

M. Staib, M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Department of Physics and Space SciencesFlorida Institute of Technology

Page 2: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Presentation Outline

• GEM detector design for ft3 MT station

• GEM stretching and framing by IR thermal method

• Gain uniformity measurements of detectors fabricated using this new method

• Future work regarding implementation of these detectors into our ft3 muon tomography station

Page 3: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Gas Electron Multiplier (GEM) Detector

V

μ-

e-

GEM foil under electron microscope (F. Sauli)

~400 V

Page 4: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

30 cm x 30 cm triple-GEM detectors for muon tomography based on design used for the COMPASS experiment at CERN and are

operated in Ar/CO2 70:30 mixture

X-Y Cartesian readout strips 1568 strips per detector

400 μm pitch

Triple-GEM Detector for MT station

COMPASS Design

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Assembled GEM Detector

Drift Cathode

GEM foil

FR4 Spacer Frame

X-Y Readout

Nucl. Inst. and Meth. A 490 (2002) 177–203

Page 5: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Traditional GEM Foil Stretching

Mechanical (INFN) Thermal (CERN/FIT)

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

• GEM foils lack mechanical rigidity and must be stretched and framed before being assembled into a detector.

• Traditional methods of tensioning the foils are expensive to implement.

• Stretching must take place under clean room conditions.

Framed GEM Foil

Page 6: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Low-Cost GEM Stretching Using IR Heating

Page 7: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Low-Cost GEM Stretching Using IR Heating

Two 30 cm x 30 cm detectors were assembled at FIT using GEM foils tensioned by IR heating

Framed GEM Foil

30 x 30 cm2 Active Area

HV Divider Board

128

Strip

Rea

dout

Con

nect

ors

Gas In

Gas Out

Page 8: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

CMS Upgrade Using GEM Detectors

Framed GEM Foil

Gas In

Potential muon upgrade at CMS using GEMs for triggering & tracking

~1 m

(A. Sharma, S. Colafranceschi)

Page 9: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Scaled-up IR Array for Large Area GEM

We have scaled up our design in order to stretch foils as large as 1 m x 0.5 m

Wedge shaped drift foil for proposed CMS endcap upgrade using GEMs in the high-η region

Page 10: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Temperature profile of Plexiglas stretching frame

Scaled-up IR Array for Large Area GEM

Page 11: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Gain Uniformity Measurement

The gain uniformity was measured using spectra obtained from a Cd-109 gamma source.

Page 12: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Why use 109Cd for Uniformity Measurements?

Copper K-line Emission

55Fe Spectrum (16 Hours) 109Cd Spectrum (1 Hour)

5.9 keV

2.9 keV

• Only about 5% of the x-rays produced by 55Fe pass through the honeycomb cover into the drift region where they can be detected.

• 55Fe measurement is very slow, impractical for a large study.

• We can observe copper K-line fluorescence from within the detector using a 109Cd source.

Page 13: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Gain Uniformity Measurement

Top Strip Uniformity GEM Detector 9

Page 14: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Gain Uniformity Measurement

Bottom Strip Uniformity GEM 9

No-peak Measurement

Page 15: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Gain Uniformity Measurement

GEM 10 Uniformity

Top Strip Uniformity Bottom Strip Uniformity

Some problems in one corner visible on both readout axes

Page 16: M. Staib , M. Abercrombie, B. Benson, K. Gnanvo, M. Hohlmann

Outline

GEM Design

GEM Stretching

IR GEM Stretching

Characterization

Future Work

Future Work

• The GEMs assembled at Florida Tech are currently en route to CERN for use in our ft3 muon tomography station.

• We are implementing full readout of all 10 detectors (~16k channels!) and will continue characterization using complete readout electronics.

• We are working with the CMS collaboration to scale up our IR stretching method for a proposed upgrade to the muon system using large area GEM detectors.


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