Bilingual edition: English is preserved and Chinese follows each unit. Terminology uses the confirmed v20260916 glossary; automated semantic review remains traceable.
中英双语版:英文原文完整保留,中文紧随对应单元;术语采用 v20260916 确认表,自动语义审校结果可追溯。

Coma

彗星

Coma is an aberration which causes rays from an off-axis point of light in the object plane to create a trailing "comet-like" blur directed away from the optic axis (for positive coma). A lens with considerable coma may produce a sharp image in the center of the field, but become increasingly blurred toward the edges. For a single lens, coma can be partially corrected by bending the lens. More complete correction can be achieved by using a combination of lenses symmetric about a central stop.

像差是一种 aberration,它使物体平面中偏离光轴的点光源的光线形成一个向光轴方向延伸的‘彗星状’模糊区域(对于正像差)。一个存在显著像差的透镜可能在场内中心产生清晰的图像,但向边缘逐渐变得模糊。对于单透镜,可以通过弯曲透镜部分地校正像差。更彻底的校正可以通过使用关于中央光阑对称的透镜组合来实现。

Hecht, 2nd Ed in Sec 6.3 on aberrations gives a careful discussion of coma. For positive coma, rays from an off-axis object through larger radii of the lens contribute a larger oval of light further from the principal focus.

Hecht 第二版第六章第三节中关于像差的讨论中,详细说明了彗差。对于正彗差,来自偏离光轴物体的光线通过透镜较大半径区域时,会形成更远离主焦点的更大光斑。

Hecht notes that a little more than half of the light in the image is in the roughly triangular region inside the large oval above, so the image fades as it expands away from the central focus. That encourages the picturing of this image as comet-like.

Coma is shape-dependent, so a lens shape can be found with zero coma for a given object distance. That lens would not be optimum for other object distances.

彗形像差与像的形状有关,因此可以找到一个在给定物距下具有零彗形像差的透镜。该透镜对于其他物距来说可能不是最优的。

Hecht指出,图像中超过一半的光位于上方较大的椭圆内部的大三角形区域,因此图像在远离中心焦点时逐渐变暗。这鼓励人们将此图像想象成彗星状。

For more versatile correction of coma, one can use a combination of two lenses, both of which are corrected for zero coma at infinite object distance. The appropriate separation of these two lenses can correct for coma at various object distances. Coma can also be corrected by an appropriately placed stop, but the placement and size of an optimum stop also depends upon the other aberrations.

Lens Aberrations
透镜像差
为了更有效地校正彗差,可以使用两个都校正了无限远物距下零彗差的透镜组合。这两个透镜适当分离可以校正不同物距下的彗差。彗差也可以通过适当放置的孔径光阑来校正,但最优孔径光阑的位置和大小也取决于其他像差。
Index

Lens concepts

Reference
Optics References

Hecht, 2nd Ed.
Sec 6.3
索引透镜概念 参考光学 参考Hecht,第二版 第6.3节
 
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Astigmatism

散光

The kind of astigmatism commonly encountered as a vision defect is a result of different lens curvatures in different planes. If the behavior of light from a point source object is examined, then for a perfect lens it should form a focused bright spot on the opposite side of the lens. But if the focal length of the lens is different for different planes of incident light, there will be no point where all the rays from the object reach a sharp focus.

常见的视力缺陷中的散光是由于不同平面中的透镜曲率不同所导致的。如果考察从点光源物体发出的光的行为,那么对于理想的透镜来说,应该在透镜的另一侧形成一个明亮的焦点。但如果透镜在不同平面中对入射光的焦距不同,就不可能存在所有光线从物体发出后都聚焦到一个清晰点的位置。

A more general type of astigmatism, which occurs for off-axis rays through any spherically ground lens, is called oblique astigmatism.

Lens Aberrations
透镜像差
一种更一般的散光类型,发生在通过任何接地透镜的偏轴光线中,称为斜向散光。
Index

Lens concepts

Reference
Jenkins & White
p 156 ff
索引透镜概念 参考 Jenkins & White p 156 ff
 
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Oblique Astigmatism

斜向散光

The kind of astigmatism commonly encountered as a vision defect is a result of different lens curvatures in different planes. But even spherical lenses that are perfectly symmetrical exhibit a type of astigmatism for light which approaches the lens from a point off the optic axis. Oblique astigmatism is an aberration of off-axis rays that causes radial and tangential lines in the object plane to focus sharply at different distances in the image space.

像差中常见的那种因不同平面的透镜曲率差异而引起的视力缺陷,是由于光线从光学轴外的点入射时,即使球面透镜完全对称,也会产生一种光行差。光行差是偏轴光线的像差,导致物体平面上的径向和切向线在像空间中聚焦于不同的距离。

This visualization of oblique astigmatism follows the treatment of Jenkins and White in their text "Fundamentals of Optics", 4th. Ed., Sec. 9.9 . Similar treatments can be found in Pedrotti & Pedrotti, Sec 5-5 and Hecht, 2nd Ed Sec 6.3 . Oblique astigmatism arises not from any asymmetry of the lens, but an asymmetry in the nature of the optical paths followed by rays in the tangential and sagittal planes. For the sagittal plane, the extreme rays are symmetric with respect to the central ray. For the tangential plane however, the pathlengths and angles of incidence on the lens surface are different for the top and bottom rays. (Some texts use the term "meridional plane" instead of tangential plane and "radial plane" instead of sagittal plane.)

The focal distance shortens relative to that for rays along the axis by an amount approximately proportional to the square of the displacement from the axis, forming a paraboloid of revolution as the object is rotated around the axis.

相对于轴线上光线的焦距,随着物体绕轴旋转,由于与轴的位移平方成比例地缩短,形成一个旋转抛物面。

Oblique astigmatism examples
斜向散光示例
Lens Aberrations
透镜像差
这种斜向散光的可视化处理遵循Jenkins和White在《光学基础》第四版第九章第九节中的论述。类似处理也可在Pedrotti & Pedrotti的第五章第五节以及Hecht第二版第六章第三节中找到。斜向散光并非源于透镜的任何不对称性,而是源于在切向平面和视向平面中,光线所遵循的光学路径的性质存在不对称性。对于视向平面,极端光线相对于中心光线是对称的。然而,对于切向平面,顶部和底部光线在透镜表面的路径长度和入射角是不同的。(某些文献使用“meridional plane”代替切向平面,使用“radial plane”代替视向平面。)
Index

Lens concepts

Reference
Optics references
索引 透镜概念 参考 指南
 
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Oblique Astigmatism Examples

斜向散光示例

Meyer-Arendt's text does a careful job of trying to visualize the effects of oblique astigmatism in Ch 1.6. If an object consists of a short line segment perpendicular to the radial line from the optic axis (like a segment tangential to a circle centered at the optic axis in the object plane), then that line segment will image sharply in the tangential image plane. If an object consists of a short segment in the sagittal plane, like a short radial segment in the object plane, it will image sharply in the sagittal image plane.

This illustration seeks to show that radial line segments will focus sharply in the sagittal image plane while tangential line segments will focus sharply in the tangential image plane. The result is that different patterns of distortion from oblique astigmatism will appear depending upon whether the plane of projection of the image is closer to the tangential or the sagittal image plane.

这张图旨在说明,径向线段会在视向像平面中聚焦得非常清晰,而切向线段则会在切向像平面中聚焦得非常清晰。结果是,根据图像平面是更接近切向像平面还是视向像平面,不同类型的斜向散光畸变模式会显现出来。

Meyer-Arendt在第1.6章中仔细地尝试可视化斜向散光的影响。如果一个物体由一条垂直于光轴径向线的短线段组成(例如,在物体平面中,该线段与以光轴为中心的圆相切),那么该线段将在切向像平面中清晰成像。如果物体由一个位于切向平面中的短段组成,例如在物体平面中是一个径向段,那么它将在切向像平面中清晰成像。

This illustration follows Meyer-Arendt's approach to showing the different types of distortion of the image by oblique astigmatism when viewed in the tangential and sagittal focus planes.

这张图展示了Meyer-Arendt的方法,通过斜向散光在切线焦点和切线焦点平面中显示图像的不同扭曲类型。

Another approach to visualizing the effects of oblique astigmatism on the image is employed by Moller, Chapter 13. For an object like the spoked wheel shown, the circumference is imaged sharply in the tangential focus plane and the radial features are imaged sharply in the sagittal focus plane. At some point in between, each image point can be represented by a "circle of least confusion" and the overall best focus for the object is obtained at that point.

Lens Aberrations
透镜像差
另一种可视化斜向散光对图像影响的方法见于Moller,第13章。对于像图中所示的辐条轮这样的物体,其圆周在切向焦点平面中成像清晰,而径向特征在视向焦点平面中成像清晰。在两者之间某个点,每个像点都可以用“最小模糊圈”来表示,而该物体的最佳聚焦点即在该点取得。
Index

Lens concepts

Reference
Meyer-Arendt
Ch 1.6 .
索引透镜概念 参考 Meyer-Arendt 第1.6章
 
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