Removal of Stratospheric O$_3$ by Radicals: In Situ Measurements of OH, HO$_2$, NO, NO$_2$, ClO, and BrO
Simultaneous in situ measurements of the concentrations of OH, HO$_2$, ClO, BrO, NO, and NO$_2$ demonstrate the predominance of odd-hydrogen and halogen free-radical catalysis in determining the rate of removal of ozone in the lower stratosphere during May 1993. A single catalytic cycle, in which th...
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Published in: | Science (American Association for the Advancement of Science) Vol. 266; no. 5184; pp. 398 - 404 |
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Main Authors: | , , , , , , , , , , , , , , , , , , |
Format: | Journal Article |
Language: | English |
Published: |
American Society for the Advancement of Science
21-10-1994
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Subjects: | |
Online Access: | Get full text |
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Summary: | Simultaneous in situ measurements of the concentrations of OH, HO$_2$, ClO, BrO, NO, and NO$_2$ demonstrate the predominance of odd-hydrogen and halogen free-radical catalysis in determining the rate of removal of ozone in the lower stratosphere during May 1993. A single catalytic cycle, in which the rate-limiting step is the reaction of HO$_2$ with ozone, accounted for nearly one-half of the total O$_3$ removal in this region of the atmosphere. Halogen-radical chemistry was responsible for approximately one-third of the photochemical removal of O$_3$; reactions involving BrO account for one-half of this loss. Catalytic destruction by NO$_2$, which for two decades was considered to be the predominant loss process, accounted for less than 20 percent of the O$_3$ removal. The measurements demonstrate quantitatively the coupling that exists between the radical families. The concentrations of HO$_2$ and ClO are inversely correlated with those of NO and NO$_2$. The direct determination of the relative importance of the catalytic loss processes, combined with a demonstration of the reactions linking the hydrogen, halogen, and nitrogen radical concentrations, shows that in the air sampled the rate of O$_3$ removal was inversely correlated with total NO$_x$ loading. |
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ISSN: | 0036-8075 1095-9203 |
DOI: | 10.1126/science.266.5184.398 |