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Magnesium ion chemistry in the stratosphere
Authors:E.E. Ferguson  B.R. Rowe  D.W. Fahey  F.C. Fehsenfeld
Affiliation:Aeronomy Laboratory NOAA Environmental Research Laboratories, Boulder CO 80303 U.S.A.
Abstract:Laboratory measurements of reaction rate constants of magnesium ions and magnesium containing ions with O3, NO, HNO3, and H2O2 have been carried out in a flowing afterglow experiment. Mg+ ions react with O3 to produce MgO+ ions, which in turn react with O3 to produce Mg+ ions. Mg+ ions react with HNO3 and H2O2 to produce MgOH+ ions. MgOH+ ions react rapidly with HNO3 to produce NO+2 ions and Mg(HO)2. One can therefore conclude that Mg+, MgO+, or MgOH+ ions could not have significant concentrations in the stratosphere if gas phase magnesium compounds were present. The failure to observe these ions therefore cannot be used as evidence that the stratospheric magnesium, resulting from meteor ablation at higher altitudes, is in condensed phases. This is in contrast to the case for sodium where the ion chemistry is such that the failure to observe hydrated Na+ ions proves that gas phase sodium compounds are not present in the stratosphere.
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