Abstract

Precision measurements of vacuum wavelengths between 3425 and 6907 Å have been made of 95 lines in the spectrum of 86Kr from an Englehard-type lamp operated at the triple point of nitrogen. The accuracy-obtained is of the order of 0.0001 Å. The wavenumbers computed from the experimental data are consistent to 1 mK or better.

© 1964 Optical Society of America

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References

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  1. K. W. Meissner, J. Opt. Soc. Am. 31, 6405–427 (1941) (Part I);J. Opt. Soc. Am. 32, 4185–211 (1942) (Part II).
    [Crossref]
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    [Crossref]
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  5. H. Barrell, Intern. Astron. Union Commission 14 Report of the Meeting of August, 1958.
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    [Crossref]
  7. CIPM, Tech. Note, J. Opt. Soc. Am. 53, 401 (1963).
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    [Crossref]
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    [Crossref]
  10. M. J. Terrien, Compt Rend. 246, 2362–2364 (1958) (Part 2).
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    [Crossref]
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  17. V. Kaufman, IAU Commission 14 Report of the Meetings of August, 1961.

1963 (2)

1962 (3)

1961 (1)

1958 (1)

M. J. Terrien, Compt Rend. 246, 2362–2364 (1958) (Part 2).

1953 (1)

1952 (1)

C. E. Moore, Natl. Bur. Std. (U. S.) Cir. No. 467, Vol.  2 (1952).

1951 (1)

H. Barrell and P. Teasdale–Buckell, Proc. Phys. Soc. (London) B64, 413–418 (1951).

1950 (1)

1941 (1)

K. W. Meissner, J. Opt. Soc. Am. 31, 6405–427 (1941) (Part I);J. Opt. Soc. Am. 32, 4185–211 (1942) (Part II).
[Crossref]

Baird, K. M.

Barger, R. L.

Barrell, H.

H. Barrell and P. Teasdale–Buckell, Proc. Phys. Soc. (London) B64, 413–418 (1951).

H. Barrell, Intern. Astron. Union Commission 14 Report of the Meeting of August, 1958.

Edlén, B.

Erickson, K. E.

Hanes, G. R.

G. R. Hanes, D. S. Smith, K. H. Hart, and K. M. Baird (private communication, January1964).

Hart, K. H.

K. M. Baird, D. S. Smith, and K. H. Hart, J. Opt. Soc. Am. 53, 717–720 (1963).
[Crossref]

G. R. Hanes, D. S. Smith, K. H. Hart, and K. M. Baird (private communication, January1964).

Kaufman, V.

V. Kaufman, J. Opt. Soc. Am. 52, 866–870 (1962).
[Crossref]

V. Kaufman (private communication, February1964).

V. Kaufman, IAU Commission 14 Report of the Meetings of August, 1961.

V. Kaufman, Ph.D. thesis, Purdue University, August, 1959 (unpublished).

Kessler, K. G.

Meggers, W. F.

Meissner, K. W.

K. W. Meissner, J. Opt. Soc. Am. 31, 6405–427 (1941) (Part I);J. Opt. Soc. Am. 32, 4185–211 (1942) (Part II).
[Crossref]

Moore, C. E.

C. E. Moore, Natl. Bur. Std. (U. S.) Cir. No. 467, Vol.  2 (1952).

Smith, D. S.

Teasdale–Buckell, P.

H. Barrell and P. Teasdale–Buckell, Proc. Phys. Soc. (London) B64, 413–418 (1951).

Terrien, M. J.

M. J. Terrien, Compt Rend. 246, 2362–2364 (1958) (Part 2).

Compt Rend. (1)

M. J. Terrien, Compt Rend. 246, 2362–2364 (1958) (Part 2).

J. Opt. Soc. Am. (9)

Natl. Bur. Std. (U. S.) Cir. No. 467 (1)

C. E. Moore, Natl. Bur. Std. (U. S.) Cir. No. 467, Vol.  2 (1952).

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

H. Barrell and P. Teasdale–Buckell, Proc. Phys. Soc. (London) B64, 413–418 (1951).

Other (5)

V. Kaufman (private communication, February1964).

G. R. Hanes, D. S. Smith, K. H. Hart, and K. M. Baird (private communication, January1964).

V. Kaufman, IAU Commission 14 Report of the Meetings of August, 1961.

V. Kaufman, Ph.D. thesis, Purdue University, August, 1959 (unpublished).

H. Barrell, Intern. Astron. Union Commission 14 Report of the Meeting of August, 1958.

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Tables (3)

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Table I Five- and 10-cm wavelengths of 86Kr.

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Table II Consistency of the 86Kr wavelengths.

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Table III Comparison of the author’s data with the recent literature. All entries in 10−14 m.

Equations (1)

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σ = [ i = 1 n ( λ ¯ λ i ) 2 / n ] 1 2 .