A new method of differential structural analysis of gamma-family basic parameters

Details A new method of differential structural analysis of gamma-family basic parameters A new method of differential structural analysis of gamma-family basic parameters

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..396m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 396-399 (SEE N85-35848 24-93)

Astronomy and Astrophysics

Astronomy

Emulsions, Gamma Ray Bursts, Integral Equations, Maximum Likelihood Estimates, Parameterization, Photon-Electron Interaction, Structural Analysis, X Ray Imagery, Cosmic Ray Showers, Galactic Cosmic Rays, Gamma Ray Astronomy

Scientific paper

The maximum likelihood method is used for the first time to restore parameters of electron photon cascades registered on X-ray films. The method permits one to carry out a structural analysis of the gamma quanta family darkening spots independent of the gamma quanta overlapping degree, and to obtain maximum admissible accuracies in estimating the energies of the gamma quanta composing a family. The parameter estimation accuracy weakly depends on the value of the parameters themselves and exceeds by an order of the values obtained by integral methods.

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