Hydrated Positive Ions in Nitric-Oxide-Water Afterglows

W. C. Lineberger and L. J. Puckett
Phys. Rev. 187, 286 – Published 5 November 1969
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Abstract

Results of measurements performed on a stationary NO-H2O afterglow are reported in this paper. The gas mixture was contained in a large, gold-plated, cylindrical chamber in which the NO was ionized by means of krypton resonance radiation. The ions from the afterglow were sampled through an electrically insulated orifice and were quantitatively detected by time-resolved mass spectrometry. For NO+ ions reacting in NO-H2O mixtures at 295 K, the product-ion mass spectrum is dominated by NO+ and its hydrates, NO+·nH2O, and by hydrated hydronium, H3O+·nH2O. The sequence of reactions leading to these products has been determined, and the rate constant for the three-body conversion of NO+ to NO+·H2O has been measured to be (1.5 ± 0.5)×1028 cm6/sec. Bounds for several other rate constants in the reaction sequence have been obtained. The ions H3O+·2H2O, H3O+·3H2O, and H3O+·4H2O observed in the afterglow are of the same family as the hydronium ion H3O+ and its hydrates H3O+·H2O and H3O+·2H2O, which are prominent in the D region of the ionsphere. Reaction sequences similar to the one reported in this paper, which involve multiply hydrated atmospheric ions, may be an important contributors to the production of the hydrated hydronium observed in the ionosphere.

  • Received 10 June 1969

DOI:https://doi.org/10.1103/PhysRev.187.286

©1969 American Physical Society

Authors & Affiliations

W. C. Lineberger* and L. J. Puckett

  • Ballistic Research Laboratories, U. S. Army Aberdeen Research and Development Center, Aberdeen Proving Ground, Maryland 21105

  • *Present Address: Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, Colo.

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Issue

Vol. 187, Iss. 1 — November 1969

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