Laser Measurements of the H Atom + Ozone Rate Constant at Mesospheric Temperatures

Abstract

The exothermic H + O3 reaction produces OH(v) Meinel band emissions, used to derive mesospheric H concentrations and chemical heating rates. We remeasured its rate constant to reduce its uncertainty and extended the measurements to lower mesospheric temperatures using modern laser-induced fluorescence (LIF) techniques. H atoms were produced by pulsed ultraviolet laser trace photolysis of O3, followed by reaction of O((1)D) with added H2. A second, delayed, frequency-mixed dye laser measured the reaction decay rate with the remaining ozone using LIF. We monitored either the H atom decay by two photon excitation at 205 nm and detection of red fluorescence, or the OH (v = 9) product time evolution with excitation of the B(2)Σ(+)-X(2)Π (0,9) band at 237 nm and emission in the blue B(2)Σ(+)-A(2)Σ(+) (0,7) band. By cooling the enclosed low pressure flow cell we obtained measurements from 140 to 305 K at 20 to 200 Torr in Ar. Small kinetic modeling corrections were made for secondary regeneration of H atoms. The results are consistent with the current NASA JPL recommendation for this rate constant and establish its extrapolation down to the lower temperatures of the mesosphere.

A previously unrecognized source of the O 2 Atmospheric band emission in Earth’s nightglow

“…For the rate constant of the H + O 3 reaction, experimental studies by Liu et al . ( 42 ) have corroborated the most recent JPL recommendation and provided new measurements at low temperatures. The yield of OH( v = 9) from H + O 3 used in this work follows the recommendation of Adler-Golden ( 12 ), which was based on the critical evaluation by Steinfeld et al .…”