Titan's ionospheric composition and structure: Photochemical modeling of Cassini INMS data

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Titan's ionospheric composition and structure : Photochemical modeling of Cassini INMS data

Westlake, J. H. (author)

Waite, J. H., Jr. (author)

Mandt, K. E. (author)

Carrasco, N. (author)

Bell, J. M. (author)

Magee, B. A. (author)

Wahlund, Jan-Erik (author): Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen

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2012
2012
English.
In: Journal of Geophysical Research. - 0148-0227 .- 2156-2202. ; 117, s. E01003-

Related links:: https://urn.kb.se/re...; show more...; https://doi.org/10.1...; show less...

Journal article (peer-reviewed)

Abstract Subject headings

Titan's upper atmosphere produces an ionosphere at high altitudes from photoionization and electron impact that exhibits complex chemical processes in which hydrocarbons and nitrogen-containing molecules are produced through ion-molecule reactions. The structure and composition of Titan's ionosphere has been extensively investigated by the Ion and Neutral Mass Spectrometer (INMS) onboard the Cassini spacecraft. We present a detailed study using linear correlation analysis, 1-D photochemical modeling, and empirical modeling of Titan's dayside ionosphere constrained by Cassini measurements. The 1-D photochemical model is found to reproduce the primary photoionization products of N(2) and CH(4). The major ions, CH(5)(+), C(2)H(5)(+), and HCNH(+) are studied extensively to determine the primary processes controlling their production and loss. To further investigate the chemistry of Titan's ionosphere we present an empirical model of the ion densities that calculates the ion densities using the production and loss rates derived from the INMS data. We find that the chemistry included in our model sufficiently reproduces the hydrocarbon species as observed by the INMS. However, we find that the chemistry from previous models appears insufficient to accurately reproduce the nitrogen-containing organic compound abundances observed by the INMS. The major ion, HCNH(+), is found to be overproduced in both the empirical and 1-D photochemical models. We analyze the processes producing and consuming HCNH(+) in order to determine the cause of this discrepancy. We find that a significant chemical loss process is needed. We suggest that the loss process must be with one of the major components, namely C(2)H(2), C(2)H(4), or H(2).

Subject headings

NATURVETENSKAP -- Geovetenskap och miljövetenskap -- Geofysik (hsv//swe)
NATURAL SCIENCES -- Earth and Related Environmental Sciences -- Geophysics (hsv//eng)

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By the author/editor: Westlake, J. H.; Waite, J. H., Jr ...; Mandt, K. E.; Carrasco, N.; Bell, J. M.; Magee, B. A.; show more...; Wahlund, Jan-Eri ...; show less...

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NATURAL SCIENCES: NATURAL SCIENCES; and Earth and Relate ...; and Geophysics

Articles in the publication: Journal of Geoph ...

By the university: Uppsala University

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