H2O line strengths revisited: ν2 and 2ν2-ν2 at 6 μm

The necessity to revisit water spectroscopy at 6 μm was prompted by recent work indicating that some prior measurements of H₂¹⁶O line strengths (ranging through seven orders of magnitude) had larger than expected systematic errors for the stronger transitions. To investigate this, linestrengths of stronger transitions were re-measured (with 14 new H₂O spectra recorded with a Bruker 125 HR Fourier transform spectrometer at the Jet Propulsion Laboratory) and combined with re-analyzed prior results (obtained at higher optical densities from 32 spectra recorded with the FTS at Kitt Peak). Systematic differences for some of the older data sets were identified and corrected. In this paper, an internally-consistent sampling of 1243 selected line strengths are reported for (0 1 0)-(0 0 0) and (0 2 0)-(0 1 0) transitions between 783 and 2378 cm⁻¹. To confirm experimental precisions, observed and calculated line strengths are compared.     

On the Calculation of Rotational Line Strength Factors for Doublet Transitions

Abstract

The calculation of rotational line strength factors S (J) for doublet-doublet transitions is useful in many aspects of quantitative spectroscopy, since many free radical spectra involve such transitions. The important situation in which the angular momentum coupling is intermediate between Hund's cases (a) and (b) has been treated by Hill and Van Vleck¹. Their equations for S (J) form the basis of this note. The simplest type of doublet transition is ²σ(b) → ²σ(b), and these S(J) factors are given by Herzberg². Earls³ has given S(J) in simplified algebraic forms for the ²σ(b) ? ²π transition with intermediate coupling in the ²π state. A more modern derivation of the doublet S(J) factors has been given by Rubin⁴ in terms of Wigner j symbols, but it is only derived for transitions between either pure case (a) or pure case (b). The S(J) factors for transitions of higher electronic angular momentum states (Δ, φ...) with intermediate coupling, while algebraically complex, can be expressed in the form of a complicated but compact FORTRAN subroutine.     

Line positions and strengths of 41 bands including 10 OCS isotopologues in the 3850-4200 cm region

The present analysis substantially improves the spectroscopic characterization of near infrared OCS in a window region (3850-4200 cm⁻¹) important for atmospheric studies of Venus. Previous studies in this spectral region cataloged numerous OCS line positions, but accurate line intensities were measured for only three strong bands. In this paper, the corresponding line intensities are obtained for 41 OCS bands, including weak isotopic bands reported for the first time. The 2ν₃ (0002-0000) band is analyzed for 10 OCS isotopologues (adding ¹⁶O¹³C³⁴S, ¹⁷O¹²C³²S, ¹⁶O¹²C³⁶S, ¹⁸O¹²C³⁴S, and ¹⁶O¹³C³³S). In addition, observations of 0332-0330 of the main isotope, ¹⁶O¹²C³²S, provides accurate vibration-rotation parameters for the upper state (and the lower state, 0330 of ¹⁶O¹²C³²S). Finally, one unidentified band is seen at 3969.3 cm⁻¹; its lower state is clearly the ground state of ¹⁶O¹²C³²S. The line strengths of these seven previously unanalyzed bands plus 34 other bands of the OCS isotopologues, ¹⁶O¹²C³²S, ¹⁶O¹²C³⁴S, ¹⁶O¹³C³²S, ¹⁶O¹²C³³S, and ¹⁸O¹²C³²S, were least-squares fitted to determine strength parameters, S_v and Herman-Wallis coefficients. Finally, the intensities of 17 additional very weak bands were estimated to provide an extensive new database of OCS line parameters to support remote sensing of Venus. The integrated intensity in cm⁻¹/(molecule cm⁻²) at 296 K is 8.1×10⁻¹⁹ for the 3800-4200 cm⁻¹ region.