Abstract
In this paper we have discussed how the concept of passive pupil correction can be applied to improve the field performance of a ring field system. This improvement involves an optical surface coincident with the stop, or with a pupil of the system. To implement passive pupil correction, such a surface carries a non-axially symmetric asphericity that cancels aberrations along one meridian of the ring field. Because this surface is non-axially symmetric, the axial symmetry of original camera is broken and therefore the aberration compensation is not perfect for other meridians. However, an improvement of a factor of 4 can be expected if the original aberration residual consists of simple terms. The distortion characteristics of the original axially symmetric system are unchanged because the non-axially symmetric asphericity does not affect propagation of chief rays.
Original language | English (US) |
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Pages (from-to) | 658-663 |
Number of pages | 6 |
Journal | Proceedings of SPIE - The International Society for Optical Engineering |
Volume | 3482 |
DOIs | |
State | Published - Sep 21 1998 |
Externally published | Yes |
Event | International Optical Design Conference 1998 - Kona, United States Duration: Jun 8 1998 → Jun 12 1998 |
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering