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References

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  1. O. C. Jones, J. Phys. (D) 3, 1967 (1970).
  2. K. C. Lapworth, T. J. Quinn, and L. A. Allnut, J. Phys. (E) 3, 116 (1970).
  3. J. C. Flemming, Appl. Opt. 5, 195 (1966).
    [CrossRef] [PubMed]
  4. J. P. Mehltretter, Astrophysik 51, 32 (1960).
  5. D. B. Judd, J. Opt. Soc. Am. 26, 409 (1936).
    [CrossRef]
  6. T. J. Quinn and C. R. Barber, Metrologia 3, 19 (1967).
    [CrossRef]
  7. E. A. Gulbransen and W. S. Wysong, A.I.M.M.E. 175, 611 (1948).

1970 (2)

O. C. Jones, J. Phys. (D) 3, 1967 (1970).

K. C. Lapworth, T. J. Quinn, and L. A. Allnut, J. Phys. (E) 3, 116 (1970).

1967 (1)

T. J. Quinn and C. R. Barber, Metrologia 3, 19 (1967).
[CrossRef]

1966 (1)

1960 (1)

J. P. Mehltretter, Astrophysik 51, 32 (1960).

1948 (1)

E. A. Gulbransen and W. S. Wysong, A.I.M.M.E. 175, 611 (1948).

1936 (1)

Allnut, L. A.

K. C. Lapworth, T. J. Quinn, and L. A. Allnut, J. Phys. (E) 3, 116 (1970).

Barber, C. R.

T. J. Quinn and C. R. Barber, Metrologia 3, 19 (1967).
[CrossRef]

Flemming, J. C.

Gulbransen, E. A.

E. A. Gulbransen and W. S. Wysong, A.I.M.M.E. 175, 611 (1948).

Jones, O. C.

O. C. Jones, J. Phys. (D) 3, 1967 (1970).

Judd, D. B.

Lapworth, K. C.

K. C. Lapworth, T. J. Quinn, and L. A. Allnut, J. Phys. (E) 3, 116 (1970).

Mehltretter, J. P.

J. P. Mehltretter, Astrophysik 51, 32 (1960).

Quinn, T. J.

K. C. Lapworth, T. J. Quinn, and L. A. Allnut, J. Phys. (E) 3, 116 (1970).

T. J. Quinn and C. R. Barber, Metrologia 3, 19 (1967).
[CrossRef]

Wysong, W. S.

E. A. Gulbransen and W. S. Wysong, A.I.M.M.E. 175, 611 (1948).

A.I.M.M.E. (1)

E. A. Gulbransen and W. S. Wysong, A.I.M.M.E. 175, 611 (1948).

Appl. Opt. (1)

Astrophysik (1)

J. P. Mehltretter, Astrophysik 51, 32 (1960).

J. Opt. Soc. Am. (1)

J. Phys. (D) (1)

O. C. Jones, J. Phys. (D) 3, 1967 (1970).

J. Phys. (E) (1)

K. C. Lapworth, T. J. Quinn, and L. A. Allnut, J. Phys. (E) 3, 116 (1970).

Metrologia (1)

T. J. Quinn and C. R. Barber, Metrologia 3, 19 (1967).
[CrossRef]

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Figures (5)

F. 1
F. 1

Lamp-window transmittance-measurement system, (a) quartz iodine lamp, (b) neutral-density wedge, (c) interference filter, (d) 1.8-mm aperture, (e) Quinn–Barber lamp, (f) integrating sphere, and (g) photomultiplier.

F. 2
F. 2

Spectral transmittances of (a) complete aged lamp, (b) oxidized windows in series, and (c) cleaned windows in series.

F. 3
F. 3

Window-transmittance changes of a filament lamp at (a) 808, (b) 633, and (c) 448 nm, all shortly after the lamp was opened.

F. 4
F. 4

Window-transmittance changes of a filament lamp at (a) 808, (b) 633, and (c) 448 nm, several days after the lamp was opened.

F. 5
F. 5

Calculated spectral transmittances of window deposit: (a) tungsten film and (b) oxidized film.

Equations (1)

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( τ t τ 0 ) / ( τ τ 0 ) = exp ( k t α ) ,