摘要
无光焦度校正板自身无色差和像面弯曲,并具有弯曲PW和光焦度1φ1及1φ2等变数,为光学系统的像差校正提供了很大的方便。以系统通光孔径Φ=300 mm,相对孔径A=1/2,光阑位置lp2/f=-0.75,主镜为球面反射镜为例,设计了一种带有无光焦度校正板且光阑在主反射镜前的牛顿光学系统。通过对光学系统进行光线计算、像差分析和优化,得到校正板透镜最佳光焦度1φ1=5,优化后的轴上点波前像差W=0.000 1λ。
Since a zero-power corrector itself has no achromatic aberration and Petzval curvature, and has such variables as curvature PW, powers φ11 and φ12, etc, it makes the correction of the aberrations of an optical system easier. A Newton optical system with a zero-power corrector, whose stop is before the primary mirror, is proposed. The parameters of the system are the clear aperture φ=300mm, relative aperture A=1/2, stop position lp2/f=-0.75, and the eccentricity of the primary mirror e^2=0. Based on the ray calculation, aberration analysis and optimization of the optical system, the corrector lens optimal power φ11=5, and the optimized on-axis wavefront aberration W=0.0001λ, were obtained.
出处
《应用光学》
CAS
CSCD
2008年第5期753-757,共5页
Journal of Applied Optics
关键词
光学设计
牛顿光学系统
无光焦度校正板
三级像差理论
optical design
Newton optical system
zero-power corrector
third-orderaberration theory