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POST-FOCAL AND PRE-FOCAL TWO MIRROR SYSTEMS

Abstract

While investigating a potential of two-mirror systems with spherical surfaces for searching new solutions it looks rather reasonable to delineate fields of schematic solutions classifying  possible and well-known  types of systems along motion of zero ray in the system. As a result of the  investigations a classification has been made in three types of systems along motion of zero ray in an objective.

Calculation of aberration factors of 3-power has shown that systems of the first type have the highest potential  because astigmatism and curvature are corrected there in a better way that specifies objective resolution. A disadvantage of these systems is a high central screening.

About the Authors

N. K. Artiukhina
Belarusian National Technical University


E. P. Mitskevich
Belarusian National Technical University


References

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2. Михельсон, Н. Н. Оптические телескопы. Теория и конструкция / Н. Н. Михельсон. – М. : Наука, 1976.

3. Бездидько, С. Н. Исследование аберрационных характеристик зеркального объектива Кассегрена // Труды конференции «Прикладная оптика – 2002», Санкт-Петербург, 2002. –СПб., 2002. – Т. 3

4. Laikin, M. Modern lens design; Second Edition / M. Laikin, Marcel Dekker, Inc., 1992.


Review

For citations:


Artiukhina N.K., Mitskevich E.P. POST-FOCAL AND PRE-FOCAL TWO MIRROR SYSTEMS. Science & Technique. 2008;(5):47-50. (In Russ.)

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ISSN 2227-1031 (Print)
ISSN 2414-0392 (Online)