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The numerical method of definition of surface luminances of celestial objects on the base of mathematical modelling


In the astronomical literature the visual characteristics of celestial objects are described by visible stellar magnitude and angular sizes of object. The practice of supervision demonstrates, that the knowledge of just these characteristics it is not enough for the visibility of the object, as it is difficult to predict, what surface brightness is expected to see the object. One of optional versions of the solution of this problem is offered, which is important for the theory of pattern recognition.

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