2008
DOI: 10.1134/s0030400x08070047
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Absorption spectrum of H 3 + near 1.06 μm

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(6 citation statements)
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“…In [3], a relation of intramolecular resonances, such as Coriolis, Fermi, and Darling-Dennison resonances, with the line interference and, consequently, with the nonlinear pressure dependence of the line shift was found. That is, collisions mix to a higher extent the steady VR molecular states, which deviate significantly from the rigid top-harmonic oscillator model and whose vibrational modes are mixed.…”
Section: Introductionmentioning
confidence: 92%
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“…In [3], a relation of intramolecular resonances, such as Coriolis, Fermi, and Darling-Dennison resonances, with the line interference and, consequently, with the nonlinear pressure dependence of the line shift was found. That is, collisions mix to a higher extent the steady VR molecular states, which deviate significantly from the rigid top-harmonic oscillator model and whose vibrational modes are mixed.…”
Section: Introductionmentioning
confidence: 92%
“…Here, γ D = is the Doppler half-width at the intensity  times lower than the intensity at the line The absorption for a slant path is determined by the equation (12) where k(ν) is the profile of the corresponding line, P(h) is the pressure of the air, which depends on the altitude and the tilt angle of the path [3]. ON THE ATMOSPHERIC TRANSMISSION FOR HORIZONTAL, VERTICAL, AND SLANT ATMOSPHERIC PATHS The calculations have been performed in the spectral range 12412-12415 cm -1 , which includes two lines centered at 12414.2027 and 12413.9720 cm -1 .…”
Section: Basic Equations For a Line Profile With The Interference Takenmentioning
confidence: 99%
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