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Model of Titans ionosphere with detailed hydrocarbon ion chemistry

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TLDR
In this paper, the authors modified the previous model of Keller, et al., 1992 of the ionosphere of Titan, taking into account newly measured gas phase kinetic rates, particularly those of the higher mass hydrocarbons and nitriles.
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This article is published in Planetary and Space Science.The article was published on 1998-10-01. It has received 181 citations till now. The article focuses on the topics: Mass spectrometry.

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Ion chemistry and N-containing molecules in Titan's upper atmosphere

TL;DR: In this paper, the Ion and Neutral Mass Spectrometer (INMS) onboard the Cassini spacecraft performed the first composition measurements of Titan's ionosphere and revealed that Titan has the most compositionally complex ionosphere in the Solar System, with roughly 50 ions at or above the detection threshold.
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Current state of modeling the photochemistry of Titan's mutually dependent atmosphere and ionosphere

TL;DR: In this article, a two-stream discrete ordinates method was employed to characterize the transfer of solar radiation, and the effects of electron-impact, cosmic-ray deposition, and aerosol opacities from fractal and Mie particles.
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Atmospheric Escape and Evolution of Terrestrial Planets and Satellites

TL;DR: In this paper, the origin and evolution of Earth, Mars, Earth's, Mars' and Titan's atmospheres are discussed from the time when the active young Sun arrived at the Zero-Age-Main-Sequence.
References
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Numerical recipes

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Photochemistry of the atmosphere of Titan: comparison between model and observations.

TL;DR: The photochemistry of simple molecules containing carbon, hydrogen, nitrogen, and oxygen atoms in the atmosphere of Titan has been investigated using updated chemical schemes and the authors' own estimates of a number of key rate coefficients, which satisfactorily accounts for the concentrations of minor species observed by the Voyager IRIS and UVS instruments.
Journal ArticleDOI

Solar photo rates for planetary atmospheres and atmospheric pollutants

TL;DR: In this article, the rate coefficients and excess energies for dissociation, ionization, and dissociative ionization are presented for atomic and molecular species that have been identified or are suspected to exist in the atmospheres of planets, satellites (moons), comets, or as pollutants in the Earth atmosphere.
Journal ArticleDOI

Photochemical modeling of Titan's atmosphere

TL;DR: A new photochemical model of Titan's atmosphere which includes all the important compounds and reactions in spherical geometry from the surface to 1240 km is developed and is in a closer agreement with the abundances inferred from the Voyager infrared measurements at the equator than the Yung et al. results.
Book

Atmospheres and Ionospheres of the Outer Planets and Their Satellites

TL;DR: In this paper, an attempt at summarizing our present understanding of the atmospheres and ionospheres in the outer solar system, with particular emphasis on the relevant physics and chemistry is made.
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