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Published May 2, 2019 | Supplemental Material + Published
Journal Article Open

Temperature Dependence Study of the Kinetics and Product Yields of the HO_2 + CH_3C(O)O_2 Reaction by Direct Detection of OH and HO_2 Radicals Using 2f-IR Wavelength Modulation Spectroscopy

Abstract

The HO_2 + CH_3C(O)O_2 reaction consists of three product channels: CH_3C(O)OOH + O_2 (R1a), CH_3C(O)OH + O_3 (R1b), and OH + CH_3C(O)O + O_2 (R1c). The overall rate constant (k_1) and product yields (α_(1a), α_(1b), and α_(1c)) were determined over the atmospherically-relevant temperature range of 230 - 294 K at 100 Torr in N_2. Time resolved kinetics measurements were performed in a pulsed laser photolysis experiment in a slow flow cell employing simultaneous infrared (IR) and ultraviolet (UV) absorption spectroscopy. HO_2 and CH_3C(O)O_2 were formed by Cl-atom reactions with CH_3OH and CH_3CHO, respectively. Heterodyne near- and mid-infrared (NIR and MIR) wavelength modulation spectroscopy (WMS) was employed to selectively detect HO_2 and OH radicals. Ultraviolet absorption at 225 nm and 250 nm was used to detect various peroxy radicals as well as ozone (O_3). These experimental techniques enabled direct measurements of α_(1c) and α_(1b) via time-resolved spectroscopic detection in the MIR and the UV, respectively. At each temperature, experiments were performed at various ratios of initial HO_2 and CH_3C(O)O_2 concentrations to quantify the secondary chemistry. The Arrhenius expression was found to be k1(T) = 1.38^(+1.17)_(-0.63)×10^(-12)exp[(730±170)/T] cm^(-3) molecule^(-1) s^(-1). Α_(1a) was temperature-independent while α_(1b) and α_(1c) increased and decreased, respectively, with increasing temperatures. These trends are consistent with the current recommendation by the IUPAC data evaluation. Hydrogen-bonded adducts of HO_2 with the precursors, HO_2.CH_3OH and HO_2.CH_3CHO, played a role at lower temperatures; as part of this work, kinetics of the adducts were also measured.

Additional Information

© 2019 American Chemical Society. Copyright 2018, California Institute of Technology. Received: January 15, 2019; Revised: March 14, 2019; Published: April 3, 2019. This research was carried out by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration (NASA). The authors thank the Microdevices Lab (MDL) at the Jet Propulsion Laboratory (JPL), and in particular Mathieu Fradet and Siamak Forouhar, who were responsible for the fabrication of our mid-IR OH detection laser. Finally, A.O.H. thanks the National Science Foundation (NSF), the NASA Earth and Space Science Fellowship (NESSF), and NASA's Upper Atmospheric Research Program (UARP) and Tropospheric Chemistry Program for financial support. The authors declare no competing financial interest.

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Published - acs.jpca.9b00442.pdf

Supplemental Material - jp9b00442_si_001.pdf

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Created:
August 19, 2023
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October 20, 2023