Abstract

Recordings of the spectra of argon and krypton from microwave-excited electrodeless sources have led to observation of a considerable number of previously unreported lines. These new observations comprise 30 lines of argon between 14 000 and 25 000 A, and 10 lines of krypton between 20 000 and 25 000 A. All are accounted for as transitions between known energy levels.

© 1959 Optical Society of America

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References

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  1. W. R. Sittner and E. R. Peck, J. Opt. Soc. Am. 39, 474 (1949).
    [Crossref] [PubMed]
  2. C. J. Humphreys and H. J. Kostkowski, J. Research Natl. Bur. Standards 49, 73, RP 2345 (1952).
    [Crossref]
  3. C. J. Humphreys and E. Paul, J. Opt. Soc. Am. 46, 999 (1956).
    [Crossref]
  4. G. Racah, Phys. Rev. 61, 537(L) (1942).
  5. Trans. Intern. Astron. Union IX, 201–207 (1957).
  6. Charlotte E. Moore, Atomic Energy Levels, Natl. Bur. Standards Circ. 467, I.

1957 (1)

Trans. Intern. Astron. Union IX, 201–207 (1957).

1956 (1)

1952 (1)

C. J. Humphreys and H. J. Kostkowski, J. Research Natl. Bur. Standards 49, 73, RP 2345 (1952).
[Crossref]

1949 (1)

1942 (1)

G. Racah, Phys. Rev. 61, 537(L) (1942).

Humphreys, C. J.

C. J. Humphreys and E. Paul, J. Opt. Soc. Am. 46, 999 (1956).
[Crossref]

C. J. Humphreys and H. J. Kostkowski, J. Research Natl. Bur. Standards 49, 73, RP 2345 (1952).
[Crossref]

Kostkowski, H. J.

C. J. Humphreys and H. J. Kostkowski, J. Research Natl. Bur. Standards 49, 73, RP 2345 (1952).
[Crossref]

Moore, Charlotte E.

Charlotte E. Moore, Atomic Energy Levels, Natl. Bur. Standards Circ. 467, I.

Paul, E.

Peck, E. R.

Racah, G.

G. Racah, Phys. Rev. 61, 537(L) (1942).

Sittner, W. R.

J. Opt. Soc. Am. (2)

J. Research Natl. Bur. Standards (1)

C. J. Humphreys and H. J. Kostkowski, J. Research Natl. Bur. Standards 49, 73, RP 2345 (1952).
[Crossref]

Phys. Rev. (1)

G. Racah, Phys. Rev. 61, 537(L) (1942).

Trans. Intern. Astron. Union (1)

Trans. Intern. Astron. Union IX, 201–207 (1957).

Other (1)

Charlotte E. Moore, Atomic Energy Levels, Natl. Bur. Standards Circ. 467, I.

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Tables (2)

Tables Icon

Table I Argon i newly observed lines.

Tables Icon

Table II Krypton i, newly observed lines.