Image from System Matrix系统矩阵成像
The position of the image formed by a thick lens can be found by using the system matrix. This involves multiplying a vector form of the incident vergence successively by three matrices representing (1)the refraction by the first surface, (2)the translation to the second surface, and (3) the refraction by the second surface. Those three operations can be combined to form the system matrix. The entrance vergence can then be just multiplied times the system matrix to determine the exit vergence and from that vergence, the image distance is calculated. 厚透镜所成像的位置可通过系统矩阵来确定。这涉及将入射的矢量形式的发散光依次乘以三个矩阵,分别代表(1)第一表面的折射,(2)到第二表面的平移,以及(3)第二表面的折射。这三个操作可以组合成系统矩阵。然后,入射发散光可以简单地乘以系统矩阵以确定出射发散光,从而计算出像距。
![]() The example is for a lens with index of refraction n surrounded by air (n=1). It involves the surface powers of the lens and the thickness d between the vertexes. It also involves the principal planes H1 and H2. As with most ordinary geometrical optics, it is applicable only for small angles (paraxial rays). The development also follows the cartesian sign convention. *Using the Cartesian sign convention, the object distance is typically a negative number since it points opposite to the direction of light travel. The input vergence is therefore negative (divergent). 根据笛卡尔符号约定,物体距离通常是一个负数,因为它方向与光的传播方向相反。因此,入射发散度为负数。
The equivalent power for the thick lens can be calculated from Gullstrand's equation: 厚透镜的等效功率可通过Gullstrand方程计算:
Note that the calculation does not take into account the change in lens thickness with the angle of the incoming ray. It is typical to do the calculation only for the paraxial rays where the departure from full thickness is negligible. 需要注意的是,该计算未考虑入射光线角度变化时透镜厚度的变化。通常只对近轴光线进行计算,因为偏离完整厚度的情况可以忽略不计。
此例研究空气中(空气的折射率为1)折射率为n的透镜,涉及透镜两个表面的屈光力、两顶点之间的厚度d以及主平面H₁和H₂。与通常的几何光学分析一样,这里的结论只适用于小角度的近轴光线,并采用笛卡尔符号约定。 |
Index Lens concepts Thick lens concepts 索引透镜概念 厚透镜概念 | |||
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