Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984aj.....89.1076s&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 89, July 1984, p. 1076-1081.
Astronomy and Astrophysics
Astronomy
67
Calibrating, Low Frequencies, Radio Astronomy, Radio Interferometers, Correlation, Interpolation, Penalty Function
Scientific paper
A fundamental assumption of the self-calibration/hybrid mapping techniques, which are in widespread use in aperture synthesis data reduction, is one of isoplanatism: that over any given element of the array, all incident wave fronts, regardless of their directions of arrival, are subject to the same tropospheric/ionospheric path delays. This a poor assumption in the case of a low-frequency array (operating at frequencies lower than approximately 300 MHz), because of the large field of view of such an instrument and because of the wavelength dependence of wave-front perturbation by the ionosphere. The isoplanatism assumption may be relaxed by incorporating an interpolation formula in the solution for antenna/IF phases, and the usual mapping/deconvolution techniques then must be modified in order to cope with space-variant effects. Because of the consequent increase in the number of solution parameters, a better source model, higher signal-to-noise ratio, and a larger number of array elements (than are ordinarily required in order to self-calibrate) become desirable.
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