1 / 15

GEM Foil Stretching Using a Low-Cost Infrared Heating Array

GEM Foil Stretching Using a Low-Cost Infrared Heating Array. Elizabeth Esposito Erik Maki Undergraduate Research Florida Institute of Technology, HEP Lab A FAS Annual Conference, March 2012. Overview. Purpose / Background Previous work Improvements to previous work Results

lois-duke
Download Presentation

GEM Foil Stretching Using a Low-Cost Infrared Heating Array

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. GEM Foil Stretching Using a Low-Cost Infrared Heating Array Elizabeth Esposito Erik Maki Undergraduate Research Florida Institute of Technology, HEP Lab A FAS Annual Conference, March 2012

  2. Overview • Purpose / Background • Previous work • Improvements to previous work • Results • Conclusions • Future plans

  3. Purpose • Design a cost-effective, readily-implemented method of stretching GEM (gas electron multiplier) foils, improving upon previous designs. • 100cm x 50cm GEM foils stretched with this method will be used to upgrade the muon tomography station of Florida Institute of Technology’s High Energy Physics Lab A.

  4. Why Stretch GEM Foils? • GEM foils are a crucial component of detectors such as the triple GEM detector on the left. • In order to be useable, they must be uniform. • This uniformity is obtained through stretching, usually in a clean room oven.

  5. Muon Tomography Station (MTS) Below: Imaging area seen with two blocks of high-Z material. • Two 30cm x 30cm GEM detectors were built for Florida Tech’s muon tomography station using the following method. [GEM Detectors]

  6. Previous Work • Designed to stretch • 100cm x 50cm GEM foils – • scaled-up from 30cm x 30cm • design – as cost-efficiently as • possible using locally-sourced • materials. • Aluminum frame supports eight/sixteen 250W infrared heat lamps. • Used to stretch foils at 45°C - 50°C.

  7. Why 35°C? • The above GEM foil was stretched at 50°C. Note the ridging of the spacer ribs! Lower temperatures minimize / eliminate this! (CERN stretches at 37°C).

  8. Current Design • 1”-diameter aluminum rods support the frame – allows for greater versatility and mobility. Several stations can easily be set up on the same optical table. • Sixteen 125W heat lamps were used in place of the previous 250W bulbs. • Used to stretch foils at 35°C. Credit: Elizabeth Esposito, 2011

  9. Results Number of temperature measurements per bin Mean: 35.12°C RMS: 0.1669

  10. Top: Current results, 125 W bulbs RMS: 0.1669 Bottom: Previous results, 250 W bulbs RMS: 1.367 Number of temperature measurements per bin Number of temperature measurements per bin

  11. Results [Location key] Optical Table Long-Term Temperature Variation Stable plateau reached at ~3 hours

  12. Top: Unstretched 100 x 50cm …….GEM foil at ~25°C. Bottom: Stretched 100 x 50 cm GEM foil at 35°C. Note the reflection of the light bulbs in the foil!

  13. Conclusions • 125 W light bulbs provided a very uniform temperature of ~35°C. Temperature variations were minimal and did not affect the operation of the array. • Current results: RMS: 0.1669 compared w/ previous results: RMS:1.367. • Foils stretched using this method appeared to be uniformly stretched.

  14. Future Plans • Improve the methods of temperature control. • Build multiple arrays for more efficient detector construction. • Use the array to stretch 100cm x 50cm GEM foils for use in upgrading Florida Institute of Technology’s muon tomography station.

  15. Acknowledgements Research advisor: Dr. Marcus Hohlmann Previous work: Michael Staib Bryant Benson Kondo Gnanvo

More Related