Statistics of the Radiation from Astronomical Masers

Phys. Rev. A 6, 1643 – Published 1 October 1972
N. J. Evans II, R. E. Hills, O. E. H. Rydbeck, and E. Kollberg

Abstract

The results of an experimental determination of the statistical properties of radiation from OH maser sources are reported and interpreted. The radiation is found to have Gaussian statistics with no deviations greater than 1%.

DOI: http://dx.doi.org/10.1103/PhysRevA.6.1643

  • Published 1 October 1972
  • Received 15 May 1972

Authors & Affiliations

N. J. Evans II*

  • Department of Physics, University of California, Berkeley 94720

R. E. Hills

  • Radio Astronomy Laboratory, University of California, Berkeley 94720

O. E. H. Rydbeck and E. Kollberg

  • Onsala Space Observatory and Research Laboratory of Electronics, Chalmers University of Technology, Gothenberg, Sweden

  • *Work supported in part by the National Aeronautics and Space Administration Grant No. NGL 05-003-272.
  • Work supported in part by the National Science Foundation Grant No. GP 24611.
  • Partly supported by the Swedish National Science Research Council and the Swedish Council for Applied Research.

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