Artigo Revisado por pares

The Cosmic y-RAY Spectrum Between 0.3 and 25 MeV Measured on Apollo 15

1973; IOP Publishing; Volume: 181; Linguagem: Inglês

10.1086/152084

ISSN

1538-4357

Autores

J. I. Trombka, A. E. Metzger, James Arnold, J. L. Matteson, R. C. Reedy, L. E. Peterson,

Tópico(s)

Particle Detector Development and Performance

Resumo

view Abstract Citations (66) References (19) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Cosmic y-RAY Spectrum Between 0.3 and 25 MeV Measured on Apollo 15 Trombka, J. I. ; Metzger, A. E. ; Arnold, J. R. ; Matteson, J. L. ; Reedy, R. C. ; Peterson, L. E. Abstract The spectrum of the total (diffuse and discrete sources) cosmic y-ray background over the 0.3- 27 MeV range has been measured with an uncollimated NaI(Tl) scintillation counter 7.0 cm in diameter x 7.0 cm long located on a boom 7.6 m from the Apollo 15 service module. Data on cosmic y-rays were taken during Trans-Earth coast at various boom extensions, detector gains, and with the plastic anticoincidence scintillator enabled and disabled. The energy-loss spectrum at full extension with the anticoincidence enabled, corrected for monochromatic spacecraft 7-rays, is 0.18 counts (cm2 s MeV) 1 at 1 MeV, in agreement with previous measurements on the Ranger 3 and the ERS-l8. At 5 MeV, the Apollo measurement of 7 >c l0- counts (cm2 s MeV)-1 is about a factor of 5 below that determined from the ERS-18. Corrections for line contributions and spacecraft continuum at higher energies give a steep equivalent photon spectrum with a broad feature in the 1-3 MeV region. This flattening can be reduced (but not eliminated) with an estimated correction for spallation effects in the detector, leaving a spectrum which we interpret as a maximum estimate to the true cosmic photon spectrum in the 0.3-27 MeV range. At 3 MeV this limit is a factor of 3 and at 27 MeV a factor of 10 above a power law which extrapolates from measurements below 1 MeV. We have also measured a flux of 0.03 i 0.015 photons (cm2 s)-' at 0.51 MeV which may be mostly of local origin. Subject headings: cosmic rays - gamma rays Publication: The Astrophysical Journal Pub Date: May 1973 DOI: 10.1086/152084 Bibcode: 1973ApJ...181..737T full text sources ADS |

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