Corrected Cassegrain System*

Seymour Rosin

doi:10.1364/ao.3.000151

January 1, 1964Applied Optics

Corrected Cassegrain System*

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Key Points

Present an optical design modification to minimize optical aberrations in conventional Cassegrain telescope configurations.
Evaluated two-mirror Cassegrain configurations paired with corrective optical elements.
Calculated geometric optical path variations and field corrections across the focal plane.
Demonstrated qualitative reduction in off-axis aberrations across the corrected field.
Achieved an enlarged flat field of view while maintaining a compact telescope envelope.

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Implication

Optical design analysis demonstrates corrected Cassegrain configurations for reflective telescopes, suggesting improved wide-field imaging performance.

Abstract

Get PDF Email Share Share with Facebook Tweet This Post on reddit Share with LinkedIn Add to CiteULike Add to Mendeley Add to BibSonomy Get Citation Copy Citation Text Seymour Rosin, "Corrected Cassegrain System*," Appl. Opt. 3, 151-152 (1964) Export Citation BibTex Endnote (RIS) HTML Plain Text Citation alert Save article

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Seymour Rosin (1964) studied this question.

synapsesocial.com/papers/6a6f9861f44fa9f079dd0e3a https://doi.org/10.1364/ao.3.000151

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Corrected Cassegrain System*

Key Points

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Implication

Abstract

Discussion

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Corrected Cassegrain System*

Key Points

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Implication

Abstract

Discussion

Cite This Study

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