Correction of the Quadratic Light Source Dependence of the Aberration Polynomial based on the Characteristic Function of Hamilton
碩士 === 國立成功大學 === 機械工程學系碩博士班 === 100 === Nowadays the way of designing optical systems, most of people use optical design code to insert system model. For correcting aberration people set variables and what they want to optimize for, then optimize the system with the optimization tool of optical des...
| Main Authors: | , |
|---|---|
| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2012
|
| Online Access: | http://ndltd.ncl.edu.tw/handle/32525619105244978255 |
| Summary: | 碩士 === 國立成功大學 === 機械工程學系碩博士班 === 100 === Nowadays the way of designing optical systems, most of people use optical design code to insert system model. For correcting aberration people set variables and what they want to optimize for, then optimize the system with the optimization tool of optical design code. It sets many system variables and spends a lot of execution time for design result. Although the design way is very complete and effective, the basis of optical feature is wake.
This thesis takes based on optical aberration theory and discusses how to correct the quadratic light source dependence of the aberration polynomial which is based on the characteristic function of Hamilton. A connection between the mathematical model and the physical model due to the property of the aberration is built. Conditions of correcting the aberration in real physical system are found though the connection.
|
|---|