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Journal ArticleDOI

HITEMP, the high-temperature molecular spectroscopic database

TLDR
In this paper, a new molecular spectroscopic database for high-temperature modeling of the spectra of molecules in the gas phase is described, called HITEMP, which is analogous to the HITRAN database but encompasses many more bands and transitions than HitRAN for the absorbers H2O, CO2, CO, NO and OH.
Abstract
A new molecular spectroscopic database for high-temperature modeling of the spectra of molecules in the gas phase is described. This database, called HITEMP, is analogous to the HITRAN database but encompasses many more bands and transitions than HITRAN for the absorbers H2O, CO2, CO, NO, and OH. HITEMP provides users with a powerful tool for a great many applications: astrophysics, planetary and stellar atmospheres, industrial processes, surveillance, non-local thermodynamic equilibrium problems, and investigating molecular interactions, to name a few. The sources and implementation of the spectroscopic parameters incorporated into HITEMP are discussed.

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Citations
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Journal ArticleDOI

Habitable zones around main-sequence stars: Dependence on planetary mass

TL;DR: In this article, the authors present estimates of habitable zones (HZs) around stars with stellar effective temperatures in the range 2600 K-7200 K, for planetary masses between 0.1M and 5M.
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Journal ArticleDOI

Infrared laser-absorption sensing for combustion gases

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Journal ArticleDOI

The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres

TL;DR: The ExoMol database as mentioned in this paper provides extensive line lists of molecular transitions which are valid over extended temperature ranges, including lifetimes of individual states, temperature-dependent cooling functions, Lande g-factors, partition functions, cross sections, k-coefficients and transition dipoles with phase relations.
References
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Journal ArticleDOI

Reinvestigation of the vacuum ultraviolet spectrum of CO and isotopic species: The B1Σ+ ↔ X1Σ+ transition

TL;DR: In this article, the B-X(2-0) band was shown to be the B(v = 0, 1, 2) level and the mass independent Dunham coefficients and equilibrium constants were derived from simultaneous least-squares fits of the absorption and emission data pertaining to each of these vibrational levels.
Journal ArticleDOI

Current updates of the water-vapor line list in HITRAN: A new “Diet” for air-broadened half-widths

TL;DR: The current edition of the HITRAN compilation employed a sophisticated algorithm for combining measurements available for the air-broadened halfwidths of water-vapor absorption lines with theoretical values as mentioned in this paper.
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Theoretical transition probabilities for the OH Meinel system.

TL;DR: The authors present a new potential energy curve, electric dipole moment function, and spin-orbit coupling function for OH in the X 2Pi state, based on high-level ab initio calculations, which give the best agreement with experimental data to date.
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H2O in stellar atmospheres

TL;DR: In this article, a detailed ab initio computation of the dipole moment surface, the vibrational transition moments, and the spectral lines for the water molecule was performed, where a total of 412 vibrational eigenstates were identified below 30 000 cm-1, corresponding to ≈ 85 000 vibrational transitions.
Journal ArticleDOI

A New Analysis of the OH Radical Spectrum from Solar Infrared Observations

TL;DR: In this paper, the authors used the solar spectrum to discover OH lines with high rotational quantum numbers, which do not appear on laboratory spectra, among which about 400 were observed for the first time.
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