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Applied Optics

Applied Optics

APPLICATIONS-CENTERED RESEARCH IN OPTICS

  • Vol. 24, Iss. 2 — Jan. 15, 1985
  • pp: 293–295

Photomultiplier dark pulses

Ralph Burnham and Donald Scarl  »View Author Affiliations


Applied Optics, Vol. 24, Issue 2, pp. 293-295 (1985)
http://dx.doi.org/10.1364/AO.24.000293


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Abstract

Dark pulse distributions from three types of photomultiplier have been fitted to Poisson distributions, both for pulses originated by single electrons and for larger pulses. These distributions can be used to determine the first-dynode secondary-emission coefficients, the fraction of electrons that create positive ions, the number of secondary electrons created by each positive ion, and the rate of output pulses above a fixed discriminator level.

© 1985 Optical Society of America

History
Original Manuscript: August 16, 1984
Published: January 15, 1985

Citation
Ralph Burnham and Donald Scarl, "Photomultiplier dark pulses," Appl. Opt. 24, 293-295 (1985)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-24-2-293


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References

  1. P. B. Coates, “Noise Sources in the C31000D Photomultiplier,” J. Phys. E 4, 201 (1971). [CrossRef]
  2. R. W. Engstrom, RCA Photomultiplier Handbook (RCA, 1980), Appendix G.
  3. B. R. Frieden, Probability, Statistical Optics, and Data Testing (Springer, New York, 1983). [CrossRef]
  4. C. C. Lo, B. Leskovar, “Afterpulse Time Spectrum Measurement of RCA 8850 Photomultiplier,” IEEE Trans. Nucl. Sci. NS-30, 445 (1983). [CrossRef]

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