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  1. E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
    [CrossRef]
  2. E. P. Chicklis, C. S. Naiman, R. C. Folweiler, J. C. Doherty, IEEE J. Quantum Electron. QE-8, 225 (1972).
    [CrossRef]
  3. O. C. Mohler, Table of Solar Spectrum Wavelengths, 11984 Å to 25578 Å (University of Michigan Press, Ann Arbor, Mich., 1955).
  4. H. D. Downing, R. H. Hunt, J. Quant. Spectrosc. Radiat. Transfer 13, 311 (1973).
    [CrossRef]
  5. Theoretical calculations of the absorption coefficient vs wavelength in the 2.06-μm region were obtained. In the laser output region they resulted in values of αc = 0.93 km−1 and αw = 0.018 km−1. Private communication, Robert Meredith, SAI, Ann Arbor, Michigan, January1974.

1973 (1)

H. D. Downing, R. H. Hunt, J. Quant. Spectrosc. Radiat. Transfer 13, 311 (1973).
[CrossRef]

1972 (1)

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, J. C. Doherty, IEEE J. Quantum Electron. QE-8, 225 (1972).
[CrossRef]

1971 (1)

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

Chicklis, E. P.

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, J. C. Doherty, IEEE J. Quantum Electron. QE-8, 225 (1972).
[CrossRef]

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

Doherty, J. C.

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, J. C. Doherty, IEEE J. Quantum Electron. QE-8, 225 (1972).
[CrossRef]

Downing, H. D.

H. D. Downing, R. H. Hunt, J. Quant. Spectrosc. Radiat. Transfer 13, 311 (1973).
[CrossRef]

Folweiler, R. C.

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, J. C. Doherty, IEEE J. Quantum Electron. QE-8, 225 (1972).
[CrossRef]

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

Gabbe, D. R.

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

Hunt, R. H.

H. D. Downing, R. H. Hunt, J. Quant. Spectrosc. Radiat. Transfer 13, 311 (1973).
[CrossRef]

Jenssen, H. P.

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

Linz, A.

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

Meredith, Robert

Theoretical calculations of the absorption coefficient vs wavelength in the 2.06-μm region were obtained. In the laser output region they resulted in values of αc = 0.93 km−1 and αw = 0.018 km−1. Private communication, Robert Meredith, SAI, Ann Arbor, Michigan, January1974.

Mohler, O. C.

O. C. Mohler, Table of Solar Spectrum Wavelengths, 11984 Å to 25578 Å (University of Michigan Press, Ann Arbor, Mich., 1955).

Naiman, C. S.

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, J. C. Doherty, IEEE J. Quantum Electron. QE-8, 225 (1972).
[CrossRef]

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

Appl. Phys. Lett. (1)

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, D. R. Gabbe, H. P. Jenssen, A. Linz, Appl. Phys. Lett. 19, 119 (1971).
[CrossRef]

IEEE J. Quantum Electron. (1)

E. P. Chicklis, C. S. Naiman, R. C. Folweiler, J. C. Doherty, IEEE J. Quantum Electron. QE-8, 225 (1972).
[CrossRef]

J. Quant. Spectrosc. Radiat. Transfer (1)

H. D. Downing, R. H. Hunt, J. Quant. Spectrosc. Radiat. Transfer 13, 311 (1973).
[CrossRef]

Other (2)

Theoretical calculations of the absorption coefficient vs wavelength in the 2.06-μm region were obtained. In the laser output region they resulted in values of αc = 0.93 km−1 and αw = 0.018 km−1. Private communication, Robert Meredith, SAI, Ann Arbor, Michigan, January1974.

O. C. Mohler, Table of Solar Spectrum Wavelengths, 11984 Å to 25578 Å (University of Michigan Press, Ann Arbor, Mich., 1955).

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Figures (3)

Fig. 1
Fig. 1

Experimental arrangement for holmium laser spectral characteristics and CO2 absorption tests: B, beam splitters; D, spectrometer detectors; R, cell input detector; S, cell output detector.

Fig. 2
Fig. 2

Variation in spectral bandwidth and position of holmium laser output. Vertical dashed lines indicate position of the 04°1–00°0 CO2 absorption lines (from Ref. 3).

Fig. 3
Fig. 3

Window (bottom curve), average energy (middle curve), and line center (top curve) absorption coefficients as a function of CO2 partial pressure in Torr. Dashed lines indicate least-squares fit to experimental data and extrapolation to atmospheric concentration that is denoted by the solid vertical line.

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