1998
DOI: 10.1117/12.327146
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<title>The HITRAN molecular spectroscopic database and HAWKS (HITRAN atmospheric workstation)</title>

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Cited by 183 publications
(121 citation statements)
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“…The idler beam is extracted from the OPO cavity and directly sent into the vacuum chamber with 3 mJ/pulse energies and 0.2 cm 2 spot size area. At these intensities, H 2 O in the 1 01 rotational state has only a 5% probability 65 65 A digital delay generator provides a variable waiting time between the OPO and 193 nm excimer laser and therefore probes predissociation dynamics on time scales ranging from ∼5 ns to 1 μs. The 193 nm UV beam (15 mJ/pulse, ∼0.5 cm 2 area) selectively photolyzes the vibrationally excited H 2 O to make OH radicals, which are subsequently detected by a third LIF laser (303-310 nm, beam energy ∼2.5 mJ), obtained from frequency doubling the output of a dye laser pumped by a frequency doubled YAG laser.…”
Section: Methodsmentioning
confidence: 99%
“…The idler beam is extracted from the OPO cavity and directly sent into the vacuum chamber with 3 mJ/pulse energies and 0.2 cm 2 spot size area. At these intensities, H 2 O in the 1 01 rotational state has only a 5% probability 65 65 A digital delay generator provides a variable waiting time between the OPO and 193 nm excimer laser and therefore probes predissociation dynamics on time scales ranging from ∼5 ns to 1 μs. The 193 nm UV beam (15 mJ/pulse, ∼0.5 cm 2 area) selectively photolyzes the vibrationally excited H 2 O to make OH radicals, which are subsequently detected by a third LIF laser (303-310 nm, beam energy ∼2.5 mJ), obtained from frequency doubling the output of a dye laser pumped by a frequency doubled YAG laser.…”
Section: Methodsmentioning
confidence: 99%
“…Our prior results, used by the IPCC (4), were analytic fits to calculations with a one-dimensional radiative-convective model (17). The present results (Table 1) are based on calculations of adjusted radiative forcing (5), using the SI2000 version of the Goddard Institute for Space Studies three-dimensional climate model (8,13), with the absorption coefficients fit to line-by-line radiative transfer calculations, using current HITRAN (18) (5,6).…”
mentioning
confidence: 99%
“…This database contains individual parameters for calculating spectral lines, along with the parameters for the effect of various factors, such as temperature, pressure and the content of other components in the gas mixture, on the shape of the lines. The transmittance of a gas can be calculated as follows [39]:…”
Section: Line-by-line Modellingmentioning
confidence: 99%