Results 201 to 210 of about 19,435 (235)

High-resolution 3-micron Spectral Features of Titan Identified with Updated CH3D and C2H6 Line Lists

, 2007
Sang Joon Kim, Heeyoung Seo, J. Kim, T. R. Geballe, R. Courtin, Linda R. Brown   +5 more
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GOSAT-2009 methane spectral line list in the 5550–6236cm−1 range

Journal of Quantitative Spectroscopy and Radiative Transfer, 2010
Abstract 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, O.M. Lyulin, S.N. Mikhailenko, V.I. Perevalov, N.N. Filippov, I.M. Grigoriev, I. Morino, T. Yokota, R. Kumazawa, T. Watanabe   +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, 2016
Abstract 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, T.A. Dmitrieva, I.E. Gordon   +2 more
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List of references on spectral line analysis

Signal Processing, 1993
Abstract 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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Lithium abundances in atmospheres of carbon stars estimated with the help of modern lists of spectral lines

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, Ya. V. Pavlenko, K. Abia, A. E. Rozenbush   +3 more
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A spectral line list for water isotopologues in the 1100–4100 cm−1 region for application to CO2-rich planetary atmospheres

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, Michaella Farese, Candice L. Renaud   +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, 2023
I. A. Vasilenko, O. V. Naumenko, V.-M. Horneman   +2 more
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Accurate 14NH3 line-list for the 2.3 μm spectral region

Journal of Quantitative Spectroscopy and Radiative Transfer, 2021
P. Čermák, P. Cacciani, J. Cosléou
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Expert list of absorption lines of the ³²S¹⁶O₂ molecule in the 0-4200 cm^-¹ spectral region

Optika Atmosfery i Okeana, 2023
I.A. Vasilenko, O.V. Naumenko, V.-M. Horneman   +2 more
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EXPERIMENTAL LINE LIST OF WATER VAPOR ABSORPTION LINES IN THE SPECTRAL RANGES 1850 - 2280 CM AND 2390 - 4000 CM

Proceedings of the 72nd International Symposium on Molecular Spectroscopy, 2017
Joep Loos, Georg Wagner, Manfred Birk
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