Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993avest..27...47p&link_type=abstract
Astronomicheskii Vestnik (ISSN 0320-930X), vol. 27, no. 4, p. 47-64
Astronomy and Astrophysics
Astronomy
2
Calibrating, Lunar Surface, Planetary Surfaces, Spectrophotometry, Standards, Brightness, Infrared Photometry, Light Scattering, Mathematical Models, Visual Photometry
Scientific paper
The use of the Moon and of bright planets for calibration of the spectrophotometric parameters of cosmic images is grounded. The principal condition of the calibration method in the visible (0.45 micrometer) and the far infrared (10-12 micrometer) wavelengths and requirement of the initial material for the construction of the numerical model are established. The data base of the spectrophotometric measuring of the brightness of separate points on the surface of the Moon and a numerical model of the scattered light of the lunar surface are used. The image of the Moon in the visible and IR spectrum on the IBM PC screen will be reproduced by an automatic program for the calibration and normalization of the results of photometry of terrestrial natural objects.
Novikov Victor
Pugacheva S. G.
Shevchenko Valentin
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