Hermite polynomials and one-dimensional restoration in radio astronomy

Details Hermite polynomials and one-dimensional restoration in radio astronomy Hermite polynomials and one-dimensional restoration in radio astronomy

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85..168l&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 1-2, May 1980, p. 168-173. Research supported by the Fonds National de la Recherche Sc

Astronomy and Astrophysics

Astronomy

1

Hermitian Polynomial, Radio Astronomy, Restoration, Solar Spectrometers, Signal To Noise Ratios, White Noise

Scientific paper

The paper shows that restoration in radio astronomy can be performed by series of Hermite polynomials. The formulation of the problem takes a fully linear form. Its resolution consists of the inversion of an infinite matrix which is performed using recurrence relations. The practical use of this method leads to satisfactory numerical results with short computing times; the method applies best to extended sources, like the sun, and has been tried for the E-W basis of the solar interferometer of the Royal Observatory of Belgium.

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