Image from Principal Planes主平面的图像
The thin lens equation can be used with thick lenses if the principal planes are found. The equivalent focal length of the thick lens can be found from Gullstrand's equation, and the front and back vertex focal lengths obtained. Once that is done, the principal planes can be located by subtracting the vertex focal lengths from the equivalent focal length. The equivalent focal length and the distance from first principal distance H1 to the object can be used to calculate the image distance from the second principal plane H2. From that distance, the image distance from the back vertex can be deduced. 薄透镜方程可以在找到主平面的情况下用于厚透镜。厚透镜的等效焦距可通过Gullstrand方程求得,并可获得前顶点和后顶点焦距。一旦完成这些步骤,就可以通过从等效焦距中减去顶点焦距来确定主平面的位置。等效焦距和从第一个主平面到物体的距离H1可以用来计算从第二个主平面H2到像的距离。从该距离可以推导出从后顶点到像的距离。
![]() Note that the calculation below 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. The segments in boxes below are the limiting cases where the lens thickness is taken as zero (thin lens approximation). 需要注意的是,下面的计算未考虑入射光线角度变化对透镜厚度的影响。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。下面方框中的段落是极限情况,即假设透镜厚度为零(薄透镜近似)。
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Index Lens concepts Thick lens concepts Reference Meyer-Arendt 索引透镜概念 厚透镜概念 参考 Meyer-Arendt | |||||
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