Excel Files for Teaching About Wave Fronts and Rays for a Wave Moving in Media with Changing Index of Refraction

P. Mihas
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Abstract

In teaching about waves the students are learning how to find the refracted rays by using wave fronts or finding the wave fronts by using the rays. The usual teaching is based on models where the speed of the wave is constant in one medium and changes abruptly as the wave passes from one medium to another. This paper deals with ways of calculation the wave fronts and the rays for the case of a continuous changing of the index of refraction. For this purpose, Fermat’s principle is applied for multiple layers of very small thickness. Two models are presented for the speed of the waves: A model on which the wave speed depends on the square root of the depth of penetration of the wave and the other model, where the speed depends on a linear dependence. In both cases it is found that as the wave progresses it is “totally reflected”. In the case of the “square root dependence” the solution is a kind of cycloid which shows this behavior. In the linear case it is found that there is a moment where the wave is reflected, which is found by the maximum of a quantity “Z”. By using this quantity, the coordinates x and y can be calculated. As an application the refraction of the light in the atmosphere is calculated, where the dependence of the distance from the center of the earth is calculated and again the 2 models are applied. In this case the “square root” model gives a stronger deviation from the linear model. This helps the student to understand the change on the perceived position of the celestial bodies.
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关于波在折射率变化介质中运动时的波面和射线的Excel教学文件
在波的教学中,学生们正在学习如何用波阵面找到折射光线,或者用射线找到波阵面。通常的教学是基于这样的模型:波的速度在一种介质中是恒定的,当波从一种介质传播到另一种介质时,速度会突然改变。本文讨论了折射率连续变化情况下的波前和射线的计算方法。为此,费马原理应用于非常小厚度的多层。提出了两种波速模型:一种是波速取决于波穿透深度的平方根的模型,另一种是波速取决于线性依赖的模型。在这两种情况下,发现随着波的前进,它被“完全反射”。在“平方根依赖”的情况下,解是一种显示这种行为的摆线。在线性情况下,发现存在一个波被反射的力矩,该力矩由量“Z”的最大值找到。利用这个量,可以计算出坐标x和y。作为一个应用,我们计算了光在大气中的折射,其中计算了与地球中心的距离的依赖关系,并再次应用了这两个模型。在这种情况下,“平方根”模型与线性模型的偏差更大。这有助于学生理解天体感知位置的变化。
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