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  1. R. G. Newburgh, L. Heroux, H. E. Hinteregger, Appl. Opt. 1, 733(1962).
    [CrossRef]
  2. R. G. Newburgh, Appl. Opt. 2, 864 (1963).
    [CrossRef]
  3. F. Paresce, S. Kumar, C. S. Bowyer, Appl. Opt. 10, 1904 (1971).
    [CrossRef] [PubMed]
  4. J. A. R. Samson, in Techniques of Vacuum Ultraviolet Spectroscopy (Wiley, New York, 1967).
  5. J. E. Manson, Astrophys. J. 153, L191 (1968).
    [CrossRef]
  6. W. Ehrenberg, W. E. Spear, Proc. Phys. Soc. (London) B-64, 67(1951).
  7. J. E. Holliday, in Handbook of X-rays, E. F. Kaelble, Ed. (McGraw-Hill, New York, 1967).
  8. J. E. Manson, Solar Phys. 27, 107 (1972).
    [CrossRef]
  9. D. E. Bedo, H. E. Hinteregger, Japan. J. Appl. Phys. 4 (Suppl. 1), 473 (1965).
    [CrossRef]
  10. L. Heroux, J. E. Manson, H. E. Hinteregger, W. J. McMahon, J. Opt. Soc. Am. 55, 103 (1965).
    [CrossRef]
  11. R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
    [CrossRef]
  12. R. L. Kelly, Atomic Emission Lines Below 2000 Å, Hydrogen through Argon. (U. S. Government Printing Office, Washington, D.C.1968).

1972

J. E. Manson, Solar Phys. 27, 107 (1972).
[CrossRef]

1971

R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
[CrossRef]

F. Paresce, S. Kumar, C. S. Bowyer, Appl. Opt. 10, 1904 (1971).
[CrossRef] [PubMed]

1968

J. E. Manson, Astrophys. J. 153, L191 (1968).
[CrossRef]

1965

D. E. Bedo, H. E. Hinteregger, Japan. J. Appl. Phys. 4 (Suppl. 1), 473 (1965).
[CrossRef]

L. Heroux, J. E. Manson, H. E. Hinteregger, W. J. McMahon, J. Opt. Soc. Am. 55, 103 (1965).
[CrossRef]

1963

1962

1951

W. Ehrenberg, W. E. Spear, Proc. Phys. Soc. (London) B-64, 67(1951).

Bedo, D. E.

D. E. Bedo, H. E. Hinteregger, Japan. J. Appl. Phys. 4 (Suppl. 1), 473 (1965).
[CrossRef]

Bowyer, C. S.

Ehrenberg, W.

W. Ehrenberg, W. E. Spear, Proc. Phys. Soc. (London) B-64, 67(1951).

Grader, R. J.

R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
[CrossRef]

Heroux, L.

Hill, R. W.

R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
[CrossRef]

Hinteregger, H. E.

Holliday, J. E.

J. E. Holliday, in Handbook of X-rays, E. F. Kaelble, Ed. (McGraw-Hill, New York, 1967).

Kelly, R. L.

R. L. Kelly, Atomic Emission Lines Below 2000 Å, Hydrogen through Argon. (U. S. Government Printing Office, Washington, D.C.1968).

Kumar, S.

Manson, J. E.

J. E. Manson, Solar Phys. 27, 107 (1972).
[CrossRef]

J. E. Manson, Astrophys. J. 153, L191 (1968).
[CrossRef]

L. Heroux, J. E. Manson, H. E. Hinteregger, W. J. McMahon, J. Opt. Soc. Am. 55, 103 (1965).
[CrossRef]

McGoff, C. W.

R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
[CrossRef]

McMahon, W. J.

Newburgh, R. G.

Paresce, F.

Salmi, D. S.

R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
[CrossRef]

Samson, J. A. R.

J. A. R. Samson, in Techniques of Vacuum Ultraviolet Spectroscopy (Wiley, New York, 1967).

Spear, W. E.

W. Ehrenberg, W. E. Spear, Proc. Phys. Soc. (London) B-64, 67(1951).

Stoering, J. P.

R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
[CrossRef]

Appl. Opt.

Astrophys. J.

J. E. Manson, Astrophys. J. 153, L191 (1968).
[CrossRef]

J. Opt. Soc. Am.

Japan. J. Appl. Phys.

D. E. Bedo, H. E. Hinteregger, Japan. J. Appl. Phys. 4 (Suppl. 1), 473 (1965).
[CrossRef]

Proc. Phys. Soc. (London)

W. Ehrenberg, W. E. Spear, Proc. Phys. Soc. (London) B-64, 67(1951).

Rev. Sci. Instrum.

R. J. Grader, R. W. Hill, C. W. McGoff, D. S. Salmi, J. P. Stoering, Rev. Sci. Instrum. 42, 465 (1971).
[CrossRef]

Solar Phys.

J. E. Manson, Solar Phys. 27, 107 (1972).
[CrossRef]

Other

J. A. R. Samson, in Techniques of Vacuum Ultraviolet Spectroscopy (Wiley, New York, 1967).

J. E. Holliday, in Handbook of X-rays, E. F. Kaelble, Ed. (McGraw-Hill, New York, 1967).

R. L. Kelly, Atomic Emission Lines Below 2000 Å, Hydrogen through Argon. (U. S. Government Printing Office, Washington, D.C.1968).

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Figures (2)

Fig. 1
Fig. 1

The modified hollow cathode light source, with water cooled cathode. Clamps, screws, and connector details are not shown. Except for the water cooling connections, the source is cylindrically symmetric.

Fig. 2
Fig. 2

The spectrum of neon, as excited in the source shown in Fig. 1. The count rate scale at the left refers to the spectrum, and the transmission scale at the right refers to the Geiger counter window and pre-filter curves, as marked.

Equations (1)

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μ m = 1.4315 λ 1.994 cm 2 g - 1 .

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