@inbook{03deffdf467e44e1b3005e2a31f8e3e9,
title = "Dissociative Recombination in Planetary Ionospheres",
abstract = "Ionization in planetary atmospheres can be produced by solar photoionization, photoelectron impact ionization, and, in auroral regions, by impact of precipitating particles. This ionization is lost mainly in dissociative recombination (DR) of molecular ions. Although atomic ions cannot undergo DR, they can be transformed locally through ion-molecule reactions into molecular ions, or they may be transported vertically or horizontally to regions of the atmosphere where such transformations are possible.",
keywords = "High Solar Activity, Martian Atmosphere, Outer Planet, Dissociative Recombination, Altitude Profile",
author = "Fox, {Jane L.}",
year = "1993",
doi = "10.1007/978-1-4615-2976-7_21",
language = "American English",
isbn = "978-1-4613-6295-1",
series = "NATO Science Series B: Physics",
publisher = "Springer",
pages = "219--242",
booktitle = "Dissociative Recombination",
}