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References

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  1. R. Richter, Z. Instrumentenk. 45, 1 (1925).
  2. W. Ta-Hang, Proc. Phys. Soc. (London) 53, 157 (1941).
    [Crossref]
  3. A. Maréchal, Rev. Opt. 26, 257 (1947).
  4. R. Barakat and M. V. Morello, J. Opt. Soc. Am. 52, 992 (1962).
    [Crossref]

1962 (1)

1947 (1)

A. Maréchal, Rev. Opt. 26, 257 (1947).

1941 (1)

W. Ta-Hang, Proc. Phys. Soc. (London) 53, 157 (1941).
[Crossref]

1925 (1)

R. Richter, Z. Instrumentenk. 45, 1 (1925).

Barakat, R.

Maréchal, A.

A. Maréchal, Rev. Opt. 26, 257 (1947).

Morello, M. V.

Richter, R.

R. Richter, Z. Instrumentenk. 45, 1 (1925).

Ta-Hang, W.

W. Ta-Hang, Proc. Phys. Soc. (London) 53, 157 (1941).
[Crossref]

J. Opt. Soc. Am. (1)

Proc. Phys. Soc. (London) (1)

W. Ta-Hang, Proc. Phys. Soc. (London) 53, 157 (1941).
[Crossref]

Rev. Opt. (1)

A. Maréchal, Rev. Opt. 26, 257 (1947).

Z. Instrumentenk. (1)

R. Richter, Z. Instrumentenk. 45, 1 (1925).

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Figures (2)

Fig. 1
Fig. 1

Best focus for third-order spherical aberration for: (A) W4 = 0.7λ, (B) W4 = 0.9λ, (C) W4 = 1.1λ. The small circles indicate the computed values.

Fig. 2
Fig. 2

Best focus for fifth-order spherical aberration with ratio W4 = −3W6/2 for: (A) W6 = 3λ, (B) W6 = 4λ, (C) W6 = 5λ, (D) W6 = 6λ. The small circles indicate the computed values.

Equations (7)

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t ( 0 ) = | 2 0 1 e i k W ( ρ ) ρ d ρ | 2 ,
t ( 0 ) = 0 2 T ( ω ) ω d ω ,
Ω c = 1 / λ F ,
W ( ρ ) = W 4 ρ 4 + W 2 ρ 2 ,
W 2 = - W 4 .
W ( ρ ) = W 6 ρ 6 + W 4 ρ 4 + W 2 ρ 2 ,
W 4 = - 3 W 6 / 2.