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  • 1
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    Large-area pulse ionization chamber for measurement of extremely heavy cosmic rays (1971)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Large area parallel-plate pulse ionization chamber for high altitude balloon measurements of relativistic cosmic ray heavy nuclei
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: ; 331-335. (
    Format: text
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    NASA TECHNICAL REPORTS
  • 2
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    Scintillator-fiber charged-particle track-imaging detector (1983)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: A scintillator-fiber charged-particle track-imaging detector has been developed using a bundle of square cross-section plastic scintillator fiber optics, proximity focused onto an image intensified Charge Injection Device (CID) camera. Detector to beams of 15 MeV protons and relativistic Neon, Manganese, and Gold nuclei have been exposed and images of their tracks are obtained. This paper presents details of the detector technique, properties of the tracks obtained, and range measurements of 15 MeV protons stopping in the fiber bundle.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: International Cosmic Ray Conference; Aug 22, 1983 - Sep 03, 1983; Bangalore; India
    Format: text
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    NASA TECHNICAL REPORTS
  • 3
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    Detectors of ultraheavy cosmic rays (1983)
    In:  Other Sources
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    Publication Date: 2019-07-13
    Description: Ultraheavy cosmic rays have been measured by both passive and electronic detectors. These detectors are reviewed, and the requirements are given for the next major step in detector design.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: Composition and origin of cosmic rays; Advanced Study Institute; Jun 20, 1982 - Jun 30, 1982; Erice; Italy
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  • 4
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    Use of relativistic rise in ionization chambers for measurement of high energy heavy nuclei (1983)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: A balloon-borne instrument has been constructed to measure the energy spectra of cosmic-ray heavy nuclei in the range of about 0.3 to about 100 GeV/amu. It makes use of the relativistic rise portion of the Bethe-Bloch curve in ionization chambers for energy determination in the 10- to 100-GeV/amu interval. The instrument consists of six layers of dual-gap ionization chambers for energy determination above 10 GeV/amu. Charge is determined with a NE114 scintillator and a Pilot 425 plastic Cerenkov counter. A CO2 gas Cerenkov detector (1 atm; threshold of 30 GeV/amu) calibrates the ion chambers in the relativistic rise region. The main emphasis of the instrument is the determination of the change of the ratio of Iron (26) to the Iron secondaries (21-25) in the energy range of 10 to 100 GeV/amu. Preliminary data from a balloon flight in the fall of 1982 from Palestine, TX is presented.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: International Cosmic Ray Conference; Aug 22, 1983 - Sep 03, 1983; Bangalore; India
    Format: text
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    NASA TECHNICAL REPORTS
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