Published June 15, 1981 | Version v1
Journal article

The UH-nuclei cosmic ray detector on the third High Energy Astronomy Observatory

  • 1. McDonnell Douglas Research Labs., St. Louis, MO (USA)
  • 2. Washington Univ., St. Louis, MO (USA). McDonnell Center for the Space Sciences
  • 3. Washington Univ., St. Louis, MO (USA). Dept. of Physics
  • 4. Minnesota Univ., Minneapolis (USA). School of Physics and Astronomy
  • 5. California Inst. of Tech., Pasadena (USA). George W. Downs Lab. of Physics

Description

The third High Energy Astronomy Observatory satellite (HEAO-3) carries a particle telescope for the detection of highly charged cosmic ray nuclei. These nuclei, which have Z approx. >= 28, are much rarer than the lower charged nuclei in the cosmic radiation. As a consequence, this particle telescope was required to have a large collecting area as well as an ability to resolve individual elements. This paper describes the telescope, composed of large area parallel plate ionization chambers, multiwire ion chamber hodoscopes and a Cherenkov radiation detector. The resulting telescope has a total geometry factor of 59 000 cm2 sr and is capable of measuring the charges of nuclei in the range 14 approx. <= Z approx. <= 120. (orig.)

Additional details

Publishing Information

Journal Title
Nucl. Instrum. Methods Phys. Res.
Journal Volume
185
Journal Issue
1-3
Series
Nucl. Instrum. Methods Phys. Res.
Journal Page Range
415-426
ISSN
0029-554X