Paraxial Rays近轴光线
The commonly used optical expressions like the lens equation are approximations which are only valid for light rays close to the optic axis for which the approximation sinθ ≈ θ is valid. Such rays are called "paraxial rays". The validity of this approximation can be evaluated by looking at the series representation of the trigonometric functions, and this small angle approximation is used in numerous applications. ![]() This approximation sin x ≈ x reaches a 1% error at about 14 degrees. 这个近似式sin x ≈ x在约14度时误差达到1%。
常用的光学表达式,如透镜公式,是近似值,仅在光束接近光轴且满足近似关系sinθ ≈ θ时成立。这样的光束被称为“近轴光束”。可以通过观察三角函数的级数表示来评估该近似值的有效性,这种小角度近似在许多应用中都被使用。 For applications involving refraction, Snell's law is expressed in terms of the trigonometric functions: n1sinθ1 = n2sinθ2. But for small angles, Snell's law can be approximated by n1θ1 ≈ n2θ2. The approximation tanθ ≈ θ is used in developing the expression for surface power, which in turn is used in the lens-maker's equation and from that the derivation of the thin lens equation, so the paraxial approximation is used in most common geometrical optics expressions. 在涉及折射的应用中,斯涅尔定律用三角函数表示为:n₁sinθ₁ = n₂sinθ₂。但对于小角度,斯涅尔定律可以近似为n₁θ₁ ≈ n₂θ₂。在推导表面功率的表达式时,使用了tanθ ≈ θ的近似,而该表达式又用于透镜制造公式,从而推导出薄透镜方程,因此在大多数几何光学表达式中都使用了近轴近似。 |
Index Lens concepts References Jenkins & White, 4th Ed Sec 2.12 Pedrotti & Pedrotti, Sec 3-5 索引透镜概念 参考文献 Jenkins & White, 第四版 第2.12节 Pedrotti & Pedrotti, 第3-5节 | ||
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