Abstract

No abstract available.

Full Article  |  PDF Article

References

  • View by:
  • |
  • |
  • |

  1. H. Oelhaf, H. Fischer, “Measurements of Minor Constituents in the Middle Atmosphere from Infrared Limb Emission Spectra—A Feasibility Study,” Wiss. Mitt. Nr. 47, U. Muenchen, Meteorol. Institut (Feb.1983).
  2. H. Trinks, D. Offermann, G. Lange, H. Rippel, “Ebert-Fastie-Spektrometer E3,” in GIRL, Wissenschaftliche Instrumentierung, Beobachtungsprogramme und Mission, D. Lemke, K. Proetel, Eds. (Max-Planck-Institut fur Astronomie, Koenigsstuhl, D-6900 Heidelberg, 1982).
  3. E. Redemann, Ph.D. Thesis, Wissenschaftliche Mitteilungen, Meteorological Institute, U. Muenchen, in preparation.
  4. L. S. Rothman, Appl. Opt. 17, 3517 (1978);L. S. Rothman, S. A. Clough, R. A. McClatchey, L. G. Young, D. E. Snider, A. Goldman, Appl. Opt. 17507, (1978);L. S. Rothman, Appl. Opt. 20, 791 (1981);L. S. Rothman, A. Goldman, J. R. Gillis, R. H. Tipping, L. R. Brown, J. S. Margolis, A. G. Maki, L. D. G. Young, Appl. Opt. 20, 1323 (1981).
    [CrossRef] [PubMed]
  5. In the meantime a revised version of the AFGL line parameters compilation has been compiled by L. Rothman, Appl. Opt. 22, 000 (1Aug.1983).This version contains vastly improved parameters for the ν2, 2ν2 − ν2, ν1 + ν2, and ν2 + ν3 bands of ozone, which for the most part were not yet available on the previous AFGL tapes. Recent recalculations accounting for these O3 bands have shown that the effect of O3 has been somewhat underestimated by us in the IR window (810–860 cm−1) and in the region of the NO fundamental at 5.33 μm.
  6. D. E. Burch, D.A. Gryvnak, R. M. Patty, G. E. Bartky, J. Opt. Soc. Am. 59, 267 (1968).
    [CrossRef]
  7. J. Susskind, J. E. Searl, J. Quant. Spectrosc. Radiat. Transfer 18, 581 (1977).
    [CrossRef]
  8. H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

1983 (2)

In the meantime a revised version of the AFGL line parameters compilation has been compiled by L. Rothman, Appl. Opt. 22, 000 (1Aug.1983).This version contains vastly improved parameters for the ν2, 2ν2 − ν2, ν1 + ν2, and ν2 + ν3 bands of ozone, which for the most part were not yet available on the previous AFGL tapes. Recent recalculations accounting for these O3 bands have shown that the effect of O3 has been somewhat underestimated by us in the IR window (810–860 cm−1) and in the region of the NO fundamental at 5.33 μm.

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

1978 (1)

1977 (1)

J. Susskind, J. E. Searl, J. Quant. Spectrosc. Radiat. Transfer 18, 581 (1977).
[CrossRef]

1968 (1)

Bartky, G. E.

Burch, D. E.

Burkert, P.

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

Fergg, F.

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

Fischer, H.

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

H. Oelhaf, H. Fischer, “Measurements of Minor Constituents in the Middle Atmosphere from Infrared Limb Emission Spectra—A Feasibility Study,” Wiss. Mitt. Nr. 47, U. Muenchen, Meteorol. Institut (Feb.1983).

Gryvnak, D.A.

Lange, G.

H. Trinks, D. Offermann, G. Lange, H. Rippel, “Ebert-Fastie-Spektrometer E3,” in GIRL, Wissenschaftliche Instrumentierung, Beobachtungsprogramme und Mission, D. Lemke, K. Proetel, Eds. (Max-Planck-Institut fur Astronomie, Koenigsstuhl, D-6900 Heidelberg, 1982).

Oelhaf, H.

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

H. Oelhaf, H. Fischer, “Measurements of Minor Constituents in the Middle Atmosphere from Infrared Limb Emission Spectra—A Feasibility Study,” Wiss. Mitt. Nr. 47, U. Muenchen, Meteorol. Institut (Feb.1983).

Offermann, D.

H. Trinks, D. Offermann, G. Lange, H. Rippel, “Ebert-Fastie-Spektrometer E3,” in GIRL, Wissenschaftliche Instrumentierung, Beobachtungsprogramme und Mission, D. Lemke, K. Proetel, Eds. (Max-Planck-Institut fur Astronomie, Koenigsstuhl, D-6900 Heidelberg, 1982).

Patty, R. M.

Rabus, D.

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

Redemann, E.

E. Redemann, Ph.D. Thesis, Wissenschaftliche Mitteilungen, Meteorological Institute, U. Muenchen, in preparation.

Rippel, H.

H. Trinks, D. Offermann, G. Lange, H. Rippel, “Ebert-Fastie-Spektrometer E3,” in GIRL, Wissenschaftliche Instrumentierung, Beobachtungsprogramme und Mission, D. Lemke, K. Proetel, Eds. (Max-Planck-Institut fur Astronomie, Koenigsstuhl, D-6900 Heidelberg, 1982).

Rothman, L. S.

Searl, J. E.

J. Susskind, J. E. Searl, J. Quant. Spectrosc. Radiat. Transfer 18, 581 (1977).
[CrossRef]

Susskind, J.

J. Susskind, J. E. Searl, J. Quant. Spectrosc. Radiat. Transfer 18, 581 (1977).
[CrossRef]

Trinks, H.

H. Trinks, D. Offermann, G. Lange, H. Rippel, “Ebert-Fastie-Spektrometer E3,” in GIRL, Wissenschaftliche Instrumentierung, Beobachtungsprogramme und Mission, D. Lemke, K. Proetel, Eds. (Max-Planck-Institut fur Astronomie, Koenigsstuhl, D-6900 Heidelberg, 1982).

Voelker, W.

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

Appl. Opt. (2)

In the meantime a revised version of the AFGL line parameters compilation has been compiled by L. Rothman, Appl. Opt. 22, 000 (1Aug.1983).This version contains vastly improved parameters for the ν2, 2ν2 − ν2, ν1 + ν2, and ν2 + ν3 bands of ozone, which for the most part were not yet available on the previous AFGL tapes. Recent recalculations accounting for these O3 bands have shown that the effect of O3 has been somewhat underestimated by us in the IR window (810–860 cm−1) and in the region of the NO fundamental at 5.33 μm.

L. S. Rothman, Appl. Opt. 17, 3517 (1978);L. S. Rothman, S. A. Clough, R. A. McClatchey, L. G. Young, D. E. Snider, A. Goldman, Appl. Opt. 17507, (1978);L. S. Rothman, Appl. Opt. 20, 791 (1981);L. S. Rothman, A. Goldman, J. R. Gillis, R. H. Tipping, L. R. Brown, J. S. Margolis, A. G. Maki, L. D. G. Young, Appl. Opt. 20, 1323 (1981).
[CrossRef] [PubMed]

Beitr. Phys. Atm. (Contrib. Atm. Phys.) (1)

H. Fischer, F. Fergg, H. Oelhaf, D. Rabus, W. Voelker, P. Burkert, Beitr. Phys. Atm. (Contrib. Atm. Phys.) 56, 260 (1983).

J. Opt. Soc. Am. (1)

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

J. Susskind, J. E. Searl, J. Quant. Spectrosc. Radiat. Transfer 18, 581 (1977).
[CrossRef]

Other (3)

H. Oelhaf, H. Fischer, “Measurements of Minor Constituents in the Middle Atmosphere from Infrared Limb Emission Spectra—A Feasibility Study,” Wiss. Mitt. Nr. 47, U. Muenchen, Meteorol. Institut (Feb.1983).

H. Trinks, D. Offermann, G. Lange, H. Rippel, “Ebert-Fastie-Spektrometer E3,” in GIRL, Wissenschaftliche Instrumentierung, Beobachtungsprogramme und Mission, D. Lemke, K. Proetel, Eds. (Max-Planck-Institut fur Astronomie, Koenigsstuhl, D-6900 Heidelberg, 1982).

E. Redemann, Ph.D. Thesis, Wissenschaftliche Mitteilungen, Meteorological Institute, U. Muenchen, in preparation.

Cited By

OSA participates in CrossRef's Cited-By Linking service. Citing articles from OSA journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (3)

Fig. 1
Fig. 1

S*m spectra for the central part of the 6.2-μm band of NO2 and the most important interfering gases. Absorber masses correspond to a slant path with 20-km tangent height.

Fig. 2
Fig. 2

Synthetic emission spectra showing the R3, R4, and R5 lines of the 1–0 CO band and the interference by lines of H2O, N2O, and O3 at three tangent heights.

Fig. 3
Fig. 3

Altitude ranges of detectability and positions of pertinent spectral features of trace constituents for the EFS. The accuracy limit is assumed to be 20% of the mixing ratio. Dotted lines indicate the results for the O3 nighttime profile.

Tables (1)

Tables Icon

Table I Emission Spectra Presented in the Study

Metrics