Identification of enhanced absorption by 16O3 lines around 5μmm in high-resolution FTIR solar spectra

A. Goldman; A. Barbe; Vl G. Tyuterev; M. R. De Backer-Barilly; J. W. Hannigan; M. T. Coffey; C. P. Rinsland; R. D. Blatherwick

doi:10.1016/j.jqsrt.2004.10.009

Identification of enhanced absorption by ¹⁶O₃ lines around 5μmm in high-resolution FTIR solar spectra

A. Goldman, A. Barbe, Vl G. Tyuterev, M. R. De Backer-Barilly, J. W. Hannigan, M. T. Coffey, C. P. Rinsland, R. D. Blatherwick

Atmospheric Composition Remote Sensing and Prediction

Research output: Contribution to journal › Article › peer-review

5 Scopus citations

Abstract

A set of previously unpredicted ¹⁶O₃ strong absorption lines in the 5 μm region are identified for the first time in balloon-borne high-resolution (0.003 cm^-1) solar spectra. These spectral features are consistent with recent ozone laboratory spectra, and are interpreted by accidental resonance effects. Some of the lines are also observed in high-resolution ground-based spectra.

Original language	English
Pages (from-to)	241-250
Number of pages	10
Journal	Journal of Quantitative Spectroscopy and Radiative Transfer
Volume	96
Issue number	2 SPEC. ISS.
DOIs	https://doi.org/10.1016/j.jqsrt.2004.10.009
State	Published - Dec 1 2005

Keywords

Atmospheric ozone
Infrared Fourier transform spectroscopy
Solar spectra

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10.1016/j.jqsrt.2004.10.009

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Goldman, A., Barbe, A., Tyuterev, V. G., De Backer-Barilly, M. R., Hannigan, J. W., Coffey, M. T., Rinsland, C. P., & Blatherwick, R. D. (2005). Identification of enhanced absorption by ¹⁶O₃ lines around 5μmm in high-resolution FTIR solar spectra. Journal of Quantitative Spectroscopy and Radiative Transfer, 96(2 SPEC. ISS.), 241-250. https://doi.org/10.1016/j.jqsrt.2004.10.009

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title = "Identification of enhanced absorption by 16O3 lines around 5μmm in high-resolution FTIR solar spectra",

abstract = "A set of previously unpredicted 16O3 strong absorption lines in the 5 μm region are identified for the first time in balloon-borne high-resolution (0.003 cm-1) solar spectra. These spectral features are consistent with recent ozone laboratory spectra, and are interpreted by accidental resonance effects. Some of the lines are also observed in high-resolution ground-based spectra.",

keywords = "Atmospheric ozone, Infrared Fourier transform spectroscopy, Solar spectra",

author = "A. Goldman and A. Barbe and Tyuterev, \{Vl G.\} and \{De Backer-Barilly\}, \{M. R.\} and Hannigan, \{J. W.\} and Coffey, \{M. T.\} and Rinsland, \{C. P.\} and Blatherwick, \{R. D.\}",

year = "2005",

month = dec,

day = "1",

doi = "10.1016/j.jqsrt.2004.10.009",

language = "English",

volume = "96",

pages = "241--250",

journal = "Journal of Quantitative Spectroscopy and Radiative Transfer",

issn = "0022-4073",

publisher = "Elsevier Ltd",

number = "2 SPEC. ISS.",

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Goldman, A, Barbe, A, Tyuterev, VG, De Backer-Barilly, MR, Hannigan, JW, Coffey, MT, Rinsland, CP & Blatherwick, RD 2005, 'Identification of enhanced absorption by ¹⁶O₃ lines around 5μmm in high-resolution FTIR solar spectra', Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 96, no. 2 SPEC. ISS., pp. 241-250. https://doi.org/10.1016/j.jqsrt.2004.10.009

TY - JOUR

T1 - Identification of enhanced absorption by 16O3 lines around 5μmm in high-resolution FTIR solar spectra

AU - Goldman, A.

AU - Barbe, A.

AU - Tyuterev, Vl G.

AU - De Backer-Barilly, M. R.

AU - Hannigan, J. W.

AU - Coffey, M. T.

AU - Rinsland, C. P.

AU - Blatherwick, R. D.

PY - 2005/12/1

Y1 - 2005/12/1

N2 - A set of previously unpredicted 16O3 strong absorption lines in the 5 μm region are identified for the first time in balloon-borne high-resolution (0.003 cm-1) solar spectra. These spectral features are consistent with recent ozone laboratory spectra, and are interpreted by accidental resonance effects. Some of the lines are also observed in high-resolution ground-based spectra.

AB - A set of previously unpredicted 16O3 strong absorption lines in the 5 μm region are identified for the first time in balloon-borne high-resolution (0.003 cm-1) solar spectra. These spectral features are consistent with recent ozone laboratory spectra, and are interpreted by accidental resonance effects. Some of the lines are also observed in high-resolution ground-based spectra.

KW - Atmospheric ozone

KW - Infrared Fourier transform spectroscopy

KW - Solar spectra

UR - https://www.scopus.com/pages/publications/22944468193

U2 - 10.1016/j.jqsrt.2004.10.009

DO - 10.1016/j.jqsrt.2004.10.009

M3 - Article

AN - SCOPUS:22944468193

SN - 0022-4073

VL - 96

SP - 241

EP - 250

JO - Journal of Quantitative Spectroscopy and Radiative Transfer

JF - Journal of Quantitative Spectroscopy and Radiative Transfer

IS - 2 SPEC. ISS.

ER -

Identification of enhanced absorption by ¹⁶O₃ lines around 5μmm in high-resolution FTIR solar spectra

Abstract

Keywords

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