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  1. W. L. Faust, R. A. McFarlane, C. K. N. Patel, C. G. B. Garrett, Phys. Rev. 133, 1476A (1964).
    [CrossRef]
  2. C. E. Moore, Natl. Bur. Std. (U.S.) Circ. 4671949.
  3. A. L. Bloom, Appl. Phys. Letters 2, 101 (1963).
    [CrossRef]
  4. E. K. Plyler, L. R. Blaine, M. Nowak, J. Res. Natl. Bur. Std. 58, 195 (1957).
    [CrossRef]

1964

W. L. Faust, R. A. McFarlane, C. K. N. Patel, C. G. B. Garrett, Phys. Rev. 133, 1476A (1964).
[CrossRef]

1963

A. L. Bloom, Appl. Phys. Letters 2, 101 (1963).
[CrossRef]

1957

E. K. Plyler, L. R. Blaine, M. Nowak, J. Res. Natl. Bur. Std. 58, 195 (1957).
[CrossRef]

1949

C. E. Moore, Natl. Bur. Std. (U.S.) Circ. 4671949.

Blaine, L. R.

E. K. Plyler, L. R. Blaine, M. Nowak, J. Res. Natl. Bur. Std. 58, 195 (1957).
[CrossRef]

Bloom, A. L.

A. L. Bloom, Appl. Phys. Letters 2, 101 (1963).
[CrossRef]

Faust, W. L.

W. L. Faust, R. A. McFarlane, C. K. N. Patel, C. G. B. Garrett, Phys. Rev. 133, 1476A (1964).
[CrossRef]

Garrett, C. G. B.

W. L. Faust, R. A. McFarlane, C. K. N. Patel, C. G. B. Garrett, Phys. Rev. 133, 1476A (1964).
[CrossRef]

McFarlane, R. A.

W. L. Faust, R. A. McFarlane, C. K. N. Patel, C. G. B. Garrett, Phys. Rev. 133, 1476A (1964).
[CrossRef]

Moore, C. E.

C. E. Moore, Natl. Bur. Std. (U.S.) Circ. 4671949.

Nowak, M.

E. K. Plyler, L. R. Blaine, M. Nowak, J. Res. Natl. Bur. Std. 58, 195 (1957).
[CrossRef]

Patel, C. K. N.

W. L. Faust, R. A. McFarlane, C. K. N. Patel, C. G. B. Garrett, Phys. Rev. 133, 1476A (1964).
[CrossRef]

Plyler, E. K.

E. K. Plyler, L. R. Blaine, M. Nowak, J. Res. Natl. Bur. Std. 58, 195 (1957).
[CrossRef]

Appl. Phys. Letters

A. L. Bloom, Appl. Phys. Letters 2, 101 (1963).
[CrossRef]

J. Res. Natl. Bur. Std.

E. K. Plyler, L. R. Blaine, M. Nowak, J. Res. Natl. Bur. Std. 58, 195 (1957).
[CrossRef]

Natl. Bur. Std. (U.S.) Circ.

C. E. Moore, Natl. Bur. Std. (U.S.) Circ. 4671949.

Phys. Rev.

W. L. Faust, R. A. McFarlane, C. K. N. Patel, C. G. B. Garrett, Phys. Rev. 133, 1476A (1964).
[CrossRef]

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Figures (1)

Fig. 1
Fig. 1

Emission of a He–Ne laser near 3.39 μ with varying concentrations of methane gas inside the resonator. After methane was flushed into the gap between the Brewster window and reflector, spectra were taken from right to left as the methane diffused out. At high methane concentrations laser action is observed only at 2948.79 cm−1 (2). With no methane present only 2947.90 cm−1 (1) is observed. The maximum observed output power from the flat mirror end is about 2 mW in (1).

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