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WO.2 · Optical instruments, path differences and refraction

GRE · GRE Subject Test · GRE 物理 · 知识点 17

训练
17.1

光学仪器、光程差与折射

A gas cell in one arm of a Michelson interferometer 干涉仪 is crossed twice. Counting only one passage halves the inferred refractive-index change.

Prerequisites: 3, 33.

  • Calculate telescope magnification and grating resolving power 分辨本领
  • Relate Michelson fringe counts to double-pass optical path changes
  • Trace surface normals before applying Snell and reflection laws
词汇 训练
English 中文 拼音
resolving power/rɪˈzɒlvɪŋ ˈpaʊə/ 分辨本领 fēn biàn běn lǐng
interferometer 干涉仪 gān shè yí
17.2

Choose the system and model

For an ideal astronomical telescope adjusted for relaxed viewing at infinity, the objective forms its focal-plane image and the eyepiece collimates the emerging light. Lens separation is f_objective+f_eyepiece; angular magnification magnitude is f_objective/f_eyepiece. The usual two-converging-lens telescope produces an inverted image, represented by a negative signed angular magnification under a consistent convention. A finite final-image distance changes lens separation; do not use the infinity adjustment without checking the condition.

17.3

Use the governing relation

Resolving power R=λ/Δλ describes the smallest distinguishable wavelength separation near λ. For an ideal diffraction grating in order m with N illuminated slits, R=mN. This is a resolution criterion, not simply the angular position formula d sinθ=mλ. Increasing illuminated slit count sharpens the principal peaks; increasing slit spacing mainly changes their angular locations. A measured λ=600 nm and Δλ=3 nm gives R=200, independent of converting both lengths to metres because their ratio uses matching units.

17.4

Apply the conditions

Michelson interference depends on the optical path difference between the arms. If one arm contains a gas cell of geometric length L and index changes from n to 1 upon evacuation, a double passage changes path by 2L(n−1). If N fringes pass, the magnitude of this change is Nλ, so n−1=Nλ/(2L). For a moving mirror instead, displacement Δx gives path change 2Δx. Fringes count phase cycles; one fringe is one wavelength of optical path, not one wavelength of mirror motion.

17.5

Check the conclusion

Snell’s law n1 sinθ1=n2 sinθ2 uses angles from the local surface normal. Reflection has equal incoming and outgoing angles from that same normal. In a rectangular block, normals of neighbouring faces are perpendicular: an incidence angle measured from one normal is complementary to the angle of that same ray from the other. Draw the ray and normals before substitution. For incidence from index n into air, total internal reflection occurs only when sinθ>1/n; equality is the critical grazing case. A stated partly refracted ray must satisfy the transmission condition.

17.6

Worked method

A Michelson interferometer sends light twice through a gas cell of length L. Evacuation changes path by $2L(n-1)$. N fringes correspond to path change $N\lambda$.

$$n-1=\frac{N\lambda}{2L}=\frac{(120)(500\times10^{-9}\,\mathrm m)}{2(0.10\,\mathrm m)}=3.0\times10^{-4}.$$
Thus n = 1.00030. Moving a mirror is also double-pass; a fringe is not one wavelength of mirror motion.

Optical instruments, path differences and refraction: GRE original diagram
Optical instruments, path differences and refraction: original GRE teaching diagram.
17.7

Check conditions and vocabulary

Use optical path, not just geometric distance. Refraction angles are measured from the normal of the actual surface, and telescope focal-length addition assumes a final image at infinity.

resolving power: Wavelength divided by the smallest resolvable wavelength separation.

optical path length 光程: Geometric path weighted by refractive index along the ray.

词汇 训练
English 中文 拼音
optical path length/ˈɒptɪkl pæθ leŋθ/ 光程 guāng chéng

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