Astrophysics and Space Science

, Volume 37, Issue 1, pp 115–130 | Cite as

Observation of the energy spectrum of cosmic diffuse X-rays in the energy range 20 keV-4 MeV

  • Fumiyoshi Makino
Article

Abstract

Balloon observations of the cosmic diffuse component of hard X-rays were conducted with two independent directional counters in two energy bands, from 20 keV to 120 keV and from 90 keV to 4 MeV. The build-up effect of primary X-rays and the altitude dependence of atmospheric X-rays were properly taken into account in the analysis of the growth curves. These two experiments gave consistent results in the overlapping energy region. If the differential energy spectrum of the photon flux is represented by a power lawE−α, the value of α is 2.3 up to 100 keV, gradually increases to 2.8 at about 500 keV, and decreases to 2.0 thereabove. The spectrum above 300 keV is in parallel to the Apollo-15 spectrum, whereas the absolute intensity is somewhat smaller. The shape of the spectrum suggests the necessity of a multi-component theory on the origin of cosmic diffuse X-rays.

Keywords

Energy Spectrum Energy Range Growth Curve Energy Band Energy Region 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1975

Authors and Affiliations

  • Fumiyoshi Makino
    • 1
  1. 1.Dept. of PhysicsNagoya UniversityNagoyaJapan

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