Results 201 to 210 of about 181,754 (235)
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Expert List of Absorption Lines of the SO2 Molecule in the 2000–3000 cm–1 Spectral Region
Atmospheric and Oceanic Optics, 2020A detailed high-accuracy list of the SO2 molecule absorption lines was obtained in the 2000–3000 cm–1 spectral region, which is important for atmospheric applications, based on a combination of the high-accuracy data on experimental energy levels and variational calculations of the intensities of vibrational-rotational transitions.
I. A. Vasilenko +2 more
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GOSAT-2009 methane spectral line list in the 5550–6236cm−1 range
Journal of Quantitative Spectroscopy and Radiative Transfer, 2010Abstract A methane spectral line list for the 5550–6236 cm −1 range with the intensity cut off 4×10 −26 cm/molecule at 296 K is presented. The line list is based on new extensive measurements of methane spectral line parameters performed at different temperatures and pressures of methane and buffer gases N 2 , O 2 and air.
A.V. Nikitin +9 more
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Improved spectroscopic line list of methyl chloride in the 1900–2600 cm−1 spectral region
Journal of Quantitative Spectroscopy and Radiative Transfer, 2016Abstract Parameters of line positions and line intensities up to 2×10 –25 cm −1 /(molecule cm −2 ) for 12 CH 3 35 Cl and 12 CH 3 37 Cl were retrieved from the Fourier transform spectra in the range of 1900–2600 cm −1 . Line intensities were scaled with measurements from literature.
A.V. Nikitin +2 more
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List of references on spectral line analysis
Signal Processing, 1993Abstract The spectral line analysis (SLA), also called line spectrum analysis, deals with the problem of extracting information on sinusoidal signals from noise-corrupted measurements. It has numerous applications in sonar, radar, underwater surveillance, communications, geophysical exploration, speech analysis, nuclear physics and other fields.
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Kinematics and Physics of Celestial Bodies, 2011
We determine lithium abundances in atmospheres of three carbon stars from synthetic spectrum fitting in the λλ 668–674 nm range using the Li I λ 670.8 nm resonance doublet. To produce synthetic spectra, we use a modified list of atomic lines from the VALD database and three alternative line lists of CN and C2 molecules which are modifications of line ...
L. A. Yakovina +3 more
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We determine lithium abundances in atmospheres of three carbon stars from synthetic spectrum fitting in the λλ 668–674 nm range using the Li I λ 670.8 nm resonance doublet. To produce synthetic spectra, we use a modified list of atomic lines from the VALD database and three alternative line lists of CN and C2 molecules which are modifications of line ...
L. A. Yakovina +3 more
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Journal of Molecular Spectroscopy, 2016
Abstract A line list of transitions for seven isotopologues of water vapor in the 1100–4100 wavenumber range has been constructed for application to atmospheres rich in CO 2 . The quantum transitions for H 2 16 O, H 2 18 O, H 2 17 O, HD 16 O, HD 18 O, and HD 17 O are from the 2012 HITRAN database (Rothman et al., 2013) and those for D 2 16 O are ...
Robert R. Gamache +2 more
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Abstract A line list of transitions for seven isotopologues of water vapor in the 1100–4100 wavenumber range has been constructed for application to atmospheres rich in CO 2 . The quantum transitions for H 2 16 O, H 2 18 O, H 2 17 O, HD 16 O, HD 18 O, and HD 17 O are from the 2012 HITRAN database (Rothman et al., 2013) and those for D 2 16 O are ...
Robert R. Gamache +2 more
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Expert List of Absorption Lines of the 32S16O2 Molecule in the 0–4200 cm–1 Spectral Region
Atmospheric and Oceanic Optics, 2023I. A. Vasilenko +2 more
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Accurate
P. Čermák, P. Cacciani, J. Cosléou
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