Optimization of detector arrays for measuring the plasma distribution function in space

Details Optimization of detector arrays for measuring the plasma distribution function in space Optimization of detector arrays for measuring the plasma distribution function in space

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987baicz..38..297m&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 38, no. 5, 1987, p. 297-303.

Other

Distribution Functions, Plasma Diagnostics, Radiation Detectors, Space Plasmas, Hermitian Polynomial, Optimization, Particle Motion

Scientific paper

The author shows that the one-particle distribution function of plasma is best described by a set of mean values of low-order Hermite polynomials of particle velocities. He then describes how these Hermite moments are calculated from detector signals, and how the detectors should be optimized to minimize the errors in the Hermite moments. The optimization procedure can also be used with other sets of physical quantities describing the distribution function.

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