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Binary Ion-Molecule Reactions

Amongst the first ionospherically important reactions to be studied were  [Pg.17]

Their rate coefficients, k, were first measured at 300 K in the SA 91) and were both found to be gas kinetic (k 10-9cm3s-1). Subsequent FA studies at 300 K 137) confirmed these results. More recent FA measurements112,1 3 have shown that k is independent of temperature over the range 80-900 K which, on the available evidence, seems to be a general feature of fast ion-molecule reactions. The energy independence of such reactions is also evident from DT and FDT studies l21 138.  [Pg.17]

The temperature and energy dependence of the rate coefficients for most of the ground state ion-molecule reactions of E- and F-region significance have now been adequately determined147, including that for the reaction [Pg.18]

It is interesting to note that the earlier FA experiments only recognised the two major product channels in reaction (17) whereas the SIFT, which is especially valuable for the determination of product distributions, identified the minor 0+ product channel [Pg.18]

Detailed chemical models of the thermosphere have been produced by Oppenheimer et al.29 based on the satellite observations, which include estimated rate coefficients for several excited ion reactions. Much of the ionic reaction rate data derived from the AE satellite experiments has recently been reviewed by Ton and Torr36,  [Pg.19]


Binary ion-molecule reactions are indicated by thin arrows (c.t. indicates charge transfer), the radiative association reaction of C+ with H2 is indicated by the thick arrow and the dissociative recombination reactions are indicated by dashed arrows leading to the neutral molecules inside the compound brackets (e indicates free electrons). The molecules indicated in bold are known (observed) interstellar molecules. [Pg.146]

Note the generation again of NO+ and 02 as well as the ion N02. A detailed study has recently been reported of the reactions of the primary and secondary stratospheric ions with several molecules152) and of the reactions of O4 and Os with several stratospheric neutrals1 S3). It seems clear from these studies that although fast binary ion-molecule reactions are important first steps in the positive ion chemistry of the lower atmosphere, the subsequent chemistry is controlled by ternary association reactions (Sect. 3.2.3). [Pg.21]

Ferguson EE. Rate constants of thermal energy binary ion-molecule reactions of aeronomic interest. Atomic DataNucl Data Tables. 1973 12 159. ... [Pg.38]

The foregoing discussions have shown how valuable ion-molecule reactions are in probing potential energy surfaces of isomers, ABCD+, by accessing the surface with association reactions, transiently with binary reactions where essentially the (ABCD+) intermediate undergoes unimolecular decomposition, or as a product in binary reactions. In the association reactions, isomers can only be produced if they... [Pg.119]

Gas-phase ion chemistry is a broad field which has many applications and which encompasses various branches of chemistry and physics. An application that draws together many of these branches is the synthesis of molecules in interstellar clouds (Herbst). This was part of the motivation for studies on the neutralization of ions by electrons (Johnsen and Mitchell) and on isomerization in ion-neutral associations (Adams and Fisher). The results of investigations of particular aspects of ion dynamics are presented in these association studies, in studies of the intermediates of binary ion-molecule Sn2 reactions (Hase, Wang, and Peslherbe), and in those of excited states of ions and their associated neutrals (Richard, Lu, Walker, and Weisshaar). Solvation in ion-molecule reactions is discussed (Castleman) and extended to include multiply charged ions by the application of electrospray techniques (Klassen, Ho, Blades, and Kebarle). These studies also provide a wealth of information on reaction thermodynamics which is critical in determining reaction spontaneity and availability of reaction channels. More focused studies relating to the ionization process and its nature are presented in the final chapter (Harland and Vallance). [Pg.376]

Whilst the rate coefficients for many binary and ternary negative ion-molecule reactions have been acquired recently, predominantly using the FA technique (see the data compilation of Albritton115 ), many more are required if the important paths in the synthesis of the observed negative ion clusters are to be identified. Product distributions have been studied even less for negative ion-molecule reactions, principally because of experimental difficulties, yet more than one product channel is accessible in several atmospherically important reactions73, for example,... [Pg.22]

Primary charged species formed by galactic cosmic ray ionization are N 2, 0 2, O, N, and free electrons. The latter are rapidly attached to gas molecules, giving rise to simple negative ions, mostly 0"2. Subsequent ion molecule reactions of primary positive and negative ions lead to complex positive and negative cluster ions. Ultimately these are removed by ion-ion recombination involving either a binary or a ternary mechanism [33]. [Pg.106]

The answer to many questions that arise in binary collision processes lies in a knowledge of detailed potential energy surfaces which for the three atom systems are now attainable, however, at considerable effort and expense.85 Until such surfaces become available, we must rely on approximate or schematic potential energy curves constructed from empirical calculations and experimental information to interpret reactive scattering and rate data of ion-molecule reactions. [Pg.218]

Ion—molecule reactions, in which we are interested here, are binary collisions of ions (positive or negative) with neutral molecules resulting in chemical reactions, in which at least one chemical bond is ruptured or one new chemical bond is formed. This is the definition of ion—molecule reactions in a narrow but rather conventional sense. Some of the possible types of such reactions are... [Pg.293]

Chapter 1 deals with the kinetics of the dissociation of diatomic molecules and the recombination of atoms, and Chapters 2 and 3 with the reactions of atoms and radicals with molecules, abstraction (metathetical) processes and addition to double and triple bonds. Data for the reactions of metal atoms with a variety of inorganic, organic and metal organic compounds, derived from sodium flame and molecular beam techniques, are discussed in Chapter 4 and rapid substitution at labile metal ions in solution in Chapter 5. The theory of, and the experimental results for, ion-molecule reactions, i.e. chemical processes resulting from binary collisions of positive or negative ions with neutral molecules, are discussed in Chapter 6 and the reactions of solvated electrons in Chapter 7. [Pg.494]

However, the model proposed by Behr and coworkers [220, 292] cannot explain the change in the rate of electrode reactions occurring in binary mixtures of water with solvents more basic than water. Instead of a decrease of the rate with an increase of the organic component, an increase of the rate is expected for ion-transfer reactions. Experimentally such a maximum has never been observed [293]. One should also add that basic properties of solvent molecules adsorbed on the electrode surface may be quite different from those of bulk molecules. [Pg.283]

In spite of their seeming variety, theoretical approaches of different authors to the consideration of solid-state heterogeneous kinetics can be divided into two distinct groups. The first group takes account of both the step of diffusional transport of reacting particles (atoms, ions or, in exceptional cases if at all, radicals) across the bulk of a growing layer to the reaction site (a phase interface) and the step of subsequent chemical transformations with the participation of these diffusing particles and the surface atoms (ions) of the other component (or molecules of the other chemical compound of a binary multiphase system). This is the physicochemical approach, the main concepts and consequences of which were presented in the most consistent form in the works by V.I. Arkharov.1,46,47... [Pg.310]

First of all, note that the term "oxidation" is based on a historical premise that is not relevant from a more modem perspective namely, the combining of another element with oxygen to form a simple binary compounds i.e., an "oxide" similarly, the removal of oxygen atoms from an oxide molecule leaving the "reduced" element was the concept intended for the term "reduction". Although this idea works fairly well for many of the more simple interactions of oxygen with both metal and non-metal elements, a better, more comprehensive, definition that includes similar reactions with other elements, such as fluorine and chlorine, evolved that was based on the transfer of electrons from one atom (or ion) to another. [Pg.168]

If, for example, the formation of H2 molecules is computed, all possible binary reactions between different molecules, atoms, ions, photons, etc. have to be considered. This yields according to the above-mentioned definitions, a set of steady state equations which involve the rate constants and the densities of the various reactants. The latter quantities are then computed under the assumption of known rate constants. [Pg.60]


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