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Development of low cost school array device for observing wide area cosmic ray air showers

Research Project

Project/Area Number 16540263
Research Category

Grant-in-Aid for Scientific Research (C)

Allocation TypeSingle-year Grants
Section一般
Research Field Particle/Nuclear/Cosmic ray/Astro physics
Research InstitutionOsaka City University

Principal Investigator

TERAMOTO Yoshiki  Osaka City University, Graduate school of science, associate professor, 大学院・理学研究科, 助教授 (50163928)

Project Period (FY) 2004 – 2005
Project Status Completed (Fiscal Year 2005)
Budget Amount *help
¥3,600,000 (Direct Cost: ¥3,600,000)
Fiscal Year 2005: ¥1,600,000 (Direct Cost: ¥1,600,000)
Fiscal Year 2004: ¥2,000,000 (Direct Cost: ¥2,000,000)
Keywordscosmic ray detector / resistive plate chamber
Research Abstract

Low cost school array device consists of gas sealed type resistive plate chamber for detecting cosmic rays, an electronics circuit box which has trigger circuit for cosmic rays and circuits to measure pulse height, arrival time, etc, and a personal computer which perform the overall control. Among these components, the most difficult one to develop was gas sealed type resistive plate chamber. Resistive plate chamber has two types of operation modes. One is streamer mode and the other is avalanche mode. We built test chambers for both types and test the sealed type operation and how long do the chambers work. For the streamer mode chamber, we used argon, iso-butane, and tetrafluoroethane, mixture. As the result of the test, the streamer mode chamber could maintain 95% detection efficiency and no large difference of pulse height for one year. Aging effect, however, was observed since then and about 600 days of operation, glue came out. Avalanche mode signal has two orders of smaller signals, hence the effect to the electrodes and gas is small. Since the avalanche mode test chamber was built later than the streamer mode chamber, test period was shorter. The chamber keeps its performance for more than one year. Since the avalanche mode signals are smaller than the streamer mode signals and avalanche mode chamber is expected to last longer, we built the full size chamber with avalanche mode. The full size chamber is about four times larger. Since the area of the pickup electrode is much larger in the full size chamber than the test chamber, pickup noise was also much larger. To reduce the noise to an acceptable level, we had to divide the pickup electrode in to six. We have made six full size chambers so far. To complete the detector, we put those chambers into the stainless case and put connections, which we have not done yet. Electronics had been complete, which uses low cost parts to reduce the cost.

Report

(3 results)
  • 2005 Annual Research Report   Final Research Report Summary
  • 2004 Annual Research Report
  • Research Products

    (2 results)

All 2004

All Journal Article (2 results)

  • [Journal Article] Search for a high-rate mixture in the streamer mode operation2004

    • Author(s)
      E.Watanabe, et al.
    • Journal Title

      Nuclear Instruments and Methods 533

      Pages: 50-50

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      2005 Final Research Report Summary
  • [Journal Article] Search for a high-rate gas mixture in the streamer mode operation2004

    • Author(s)
      M.Watanabe, et al.
    • Journal Title

      Nuclear Instrument and Methods in Physics Research A 533

      Pages: 50-54

    • Related Report
      2004 Annual Research Report

URL: 

Published: 2004-04-01   Modified: 2016-04-21  

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