title: Termolecular ion-molecule reactions in Titan's atmosphere. IV. A search made at up to 1 micron in pure hydrocarbons.
abstract: The results of a study of ion-molecule reactions occurring in pure methane, acetylene, ethylene, ethane, propyne, propene, propane, and diacetylene at pressures up to 40 microns of pressure are reported. A variety of experimental methods are used: The standard double resonance in an ICR, for determination of the precursor ions and the modulated double resonance ejection in an ICR, for the determination of the daughter ions. The FA-SIFT technique was used for validation and examination of termolecular reactions with rate coefficients that are less than 10(-26) cm(6) s(-1). An extensive database of reaction kinetics already exists for many of these reactions. The main point of this study was the determination of the accuracy of this database and to search for any missing reactions and reaction channels that may have been omitted from earlier investigations. A specific objective of this work was to extend the study to the highest pressures possible to find out if there were any important termolecular reaction channels occurring. A new approach was used here. In the pure hydrocarbon gases the mass spectra were followed as a function of the pressure changes of the gas. An initial guess was first made using the current literature as a source of the reaction kinetics that were expected. A model of the ion abundances was produced from the solution of the partial differential equations in terms of reaction rate coefficients and initial abundances. The experimental data was fitted to the model for all of the pressures by a least squares minimization to the reaction rate coefficients and initial abundances. The reaction rate coefficients obtained from the model were then compared to the literature values. Several new channels and reactions were discovered when the modeled fits were compared to the actual data. This is all explained in the text and the implications of these results are discussed for the Titan atmosphere.
authors.affiliation: Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109-8099, USA. vicent.g.anicich@jpl.nasa.gov
authors.forename: Vincent G
authors.initials: VG
authors.lastname: Anicich
authors.forename: Paul
authors.initials: P
authors.lastname: Wilson
authors.forename: Murray J
authors.initials: MJ
authors.lastname: McEwan
mesh_terms: D001272:Atmosphere / Q000737:chemistry*; D005118:Extraterrestrial Environment; D006839:Hydrocarbons, Acyclic / Q000032:analysis*; D008962:Models, Theoretical; D010316:Particle Size; D018539:Saturn
chemical_list: D006839:Hydrocarbons, Acyclic