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References

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  1. A. A. Michelson, Astrophys. J. 8, 37 (1898);Proc. Am. Acad. Arts Sci. 35, 109 (1899).
    [CrossRef]
  2. H. Dammann, Optik (Leipzig) 53, 409 (1979).
  3. H. Dammann, Phys. Unserer Zeit 11, 83 (1980).
    [CrossRef]

1980

H. Dammann, Phys. Unserer Zeit 11, 83 (1980).
[CrossRef]

1979

H. Dammann, Optik (Leipzig) 53, 409 (1979).

1898

A. A. Michelson, Astrophys. J. 8, 37 (1898);Proc. Am. Acad. Arts Sci. 35, 109 (1899).
[CrossRef]

Dammann, H.

H. Dammann, Phys. Unserer Zeit 11, 83 (1980).
[CrossRef]

H. Dammann, Optik (Leipzig) 53, 409 (1979).

Michelson, A. A.

A. A. Michelson, Astrophys. J. 8, 37 (1898);Proc. Am. Acad. Arts Sci. 35, 109 (1899).
[CrossRef]

Astrophys. J.

A. A. Michelson, Astrophys. J. 8, 37 (1898);Proc. Am. Acad. Arts Sci. 35, 109 (1899).
[CrossRef]

Optik (Leipzig)

H. Dammann, Optik (Leipzig) 53, 409 (1979).

Phys. Unserer Zeit

H. Dammann, Phys. Unserer Zeit 11, 83 (1980).
[CrossRef]

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Figures (3)

Fig. 1
Fig. 1

Grating–prism compound (grism).

Fig. 2
Fig. 2

Compensating the deflection angles of two blazed transmission gratings.

Fig. 3
Fig. 3

Combinations of different blazed phase structures yielding digital-phase structures. The phase heights can simply be added. The resulting grating periods of the corresponding digital-phase gratings are given by |N2| · d1.

Equations (4)

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sin φ 1 = N 1 · ( λ / d 1 ) ,
sin φ 2 = N 2 ( λ / d 2 ) .
λ ( N 1 d 1 + N 2 d 2 ) = 0 , i.e. , N 1 d 1 = N 2 d 2 .
Prism + prism = direct-vision prism , Grating + prism = grism ; Michelson ' s echelon , Grating + grating = digital-phase grating .

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