Astigmatism of a spherical mirror caused by oblique ray incidence and its correction
Consider a system in which light is reflected obliquely by a spherical mirror as shown below. In this case, the focal length in the sagittal direction (red line) is r/(2cosθ), and the focal length in the tangential direction (blue line) is (r cosθ)/2 (in the paraxial region), resulting in large astigmatism.

Below, we will consider the reasons for this.
table of contents:
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Derivation of the focal length of the tangential component
First, as shown below, consider only the tangential component in a system where light is reflected obliquely by a spherical mirror.

Here, dθ and dψ are assumed to be infinitesimal quantities, and cos dθ = 1 and sin dθ = dθ are assumed to hold.
The conditions shown in the figure can be expressed as follows:

From Law of Sines,

Therefore, it was shown that the focal length in the tangential direction is (r cos θ)/2.
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Derivation of the focal length of the sagittal component
Next, as shown below, consider only the sagittal component in a system where light is reflected obliquely by a mirror.

Here, vector i is the direction vector of the incident light, vector j is the direction vector of the reflected light, and vector n is the normal vector of the reflecting surface.
The angle dφ is assumed to be very small.
Each direction vector is expressed as follows:

Substituting ① and ② into ③,

Moreover, the vectors between each point are expressed as follows:

Here, k is a positive real number,

If we substitute ③' and ⑥ into this and compare the y components, we get

Substituting ③' and ⑧ into ⑦, we get

Compare this with ⑥

Therefore, from ⑤,

Here, since d𝜑 is an infinitesimal quantity, cos d𝜑 ≅ 1,

Therefore, it was shown that the focal length in sagittal direction is r/(2cosθ).
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Toroidal surface shape for astigmatism correction
So far, we have treated the reflecting surface as a spherical surface, but here we consider a toroidal surface, which has a shape with different radii of curvature in the tangential and sagittal directions.
The toroidal surface can be illustrated as follows:

In this case, the shape of the toroidal surface can be expressed by the following formula [1] [2]:

where:
Tangential radius of curvature: R t = r/cosθ
Sagittal radius of curvature: R s = r cosθ
Then, the focal length in both the tangential and sagittal directions is r/2, which is the same, and astigmatism can be eliminated.
However, the aberration that occurs when light is incident obliquely on a spherical mirror is not just astigmatism; coma aberration also becomes a problem. One way to correct this is to use multiple mirrors to cancel out the coma aberration that occurs in each mirror. Czerny-Turner spectrometers are designed based on this concept.
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Related Topics
The vector relationships between incident light, reflected light, and the normal are derived in detail at the following link.
We have discussed astigmatism of reflected light caused by oblique incidence onto a mirror, and a similar phenomenon, astigmatism of refracted light caused by oblique incidence onto a parallel plane, is also discussed below.
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References
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Related literature
[A] Born, M. & Wolf, E., Principles of Optics, Cambridge University Press.
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Update History
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2025-09 Significantly revised the diagram explaining tangential components.
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2025-09 Added "Toroidal surface shape for astigmatism correction"
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2025-04 Newly released on 2025-04
