Thin Lens Equation薄透镜公式
A common Gaussian form of the lens equation is shown below. This is the form used in most introductory textbooks. A form using the Cartesian sign convention is often used in more advanced texts because of advantages with multiple-lens systems and more complex optical instruments. Either form can be used with positive or negative lenses and predicts the formation of both real and virtual images. It is valid only for paraxial rays (rays close to the optic axis) and does not apply to thick lenses. 一种常见的高斯形式的透镜公式如下所示。这是大多数入门教材中使用的形式。在更高级的教材中,常常使用笛卡尔符号约定,因为这种形式在多透镜系统和更复杂的光学仪器中具有优势。无论是哪种形式,都可以用于正透镜或负透镜,并能预测实像和虚像的形成。该公式仅适用于近轴光线(接近光轴的光线),不适用于厚透镜。
![]() If the lens equation yields a negative image distance, then the image is a virtual image on the same side of the lens as the object. If it yields a negative focal length, then the lens is a diverging lens rather than the converging lens in the illustration. The lens equation can be used to calculate the image distance for either real or virtual images and for either positive on negative lenses. The linear magnification relationship allows you to predict the size of the image. 如果透镜公式得出负的像距,则像为虚像,位于透镜与物体同侧。如果得出负的焦距,则透镜为发散透镜,而非示意图中的会聚透镜。透镜公式可用于计算实像或虚像的像距,以及用于正透镜或负透镜。线性放大率关系允许你预测像的大小。
在下方输入数据,然后点击活动公式中您希望计算的量。 |
Index Lens concepts 棱镜概念索引 | ||
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Thin-Lens Equation:Cartesian Convention薄透镜公式:笛卡尔约定
If the Cartesian sign convention is used, the Gaussian form of the lens equation becomes 如果使用笛卡尔符号约定,高斯形式的透镜公式变为
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因为在这种惯例中,量的正方向始终是光传播的方向。物体距离 o 是一个负数,因为从透镜到物体的传播方向与光的传播方向相反。薄透镜公式也可以以牛顿形式表达。高斯形式的推导基于三角几何。对于薄透镜,透镜的功率 P 是两个表面的功率之和。对于较厚的透镜,可以使用 Gullstrand 的方程来得到等效功率。 |
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Cartesian Sign Convention笛卡尔符号约定
Because the direction of light travel is consistent and there is a consistent convention to determine the sign of all distances in a calculation, this sign convention is used in many texts. It has some advantages when dealing with multilens systems and more complex optical instruments. 由于光的传播方向一致,且在计算中确定所有距离符号的惯例一致,因此这种符号约定被许多教材采用。它在处理多透镜系统和更复杂的光学仪器时具有一些优势。
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Index Lens concepts Meyer-Arendt, 2nd Ed Sec 1.3 索引透镜概念 Meyer-Arendt,第二版第1.3节 | |||
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Thin-Lens Equation:Newtonian Form薄透镜公式(牛顿形式)
In the Newtonian form of the lens equation, the distances from the focal length points to the object and image are used rather than the distances from the lens. 在牛顿形式的透镜公式中,使用的是从焦点到物体和像的距离,而不是从透镜到物体和像的距离。
![]() Newton used the "extrafocal distances" xo and xi in his formulation of the thin lens equation. It is an equivalent treatment, but the Gaussian form will be used in this resource.
牛顿使用了"额外焦点距离"x o和x i来表述薄透镜公式。这是一种等效的处理方式,但本资源将采用高斯形式。 |
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