摘要
光学仪器要求系统成像尽可能地消除球面像差和色差.应用薄透镜初级球差的理论,从数学上分析证明惠更斯目镜中场镜与视镜取平凸透镜为最佳形状,使系统成像的球面像差为最小.
Optical instruments require system imaging to eliminate spherical aberration in so far as possible. Mathe matical analysis based on the theory of the primary spherical aberration of a thin lens proves that the field lens and ocular lens of Huygens' eyepiece take the plane convex lens as the optimum shape, and as a result, the spherical aberration of system imaging is the minimum.
出处
《高师理科学刊》
2013年第5期44-47,共4页
Journal of Science of Teachers'College and University
关键词
惠更斯目镜
初级球差
极值
Huygens' eyepiece
primary spherical aberrations
extreme value