An empirical approach to modeling ion production rates in Titan's ionosphere I: Ion production rates on the dayside and globally

Author:

Richard M. S.12,Cravens T. E.1,Wylie C.1,Webb D.1,Chediak Q.1,Perryman R.3,Mandt K.3,Westlake J.4,Waite J. H.3,Robertson I.1,Magee B. A.3,Edberg N. J. T.5

Affiliation:

1. Department of Physics and Astronomy; University of Kansas; Lawrence Kansas USA

2. Department of Physics and Astronomy; Benedictine College; Atchison Kansas USA

3. Space Science and Engineering Division; Southwest Research Institute; San Antonio Texas USA

4. Johns Hopkins University Applied Physics Laboratory; Laurel Maryland USA

5. Swedish Institute of Space Physics; Uppsala Sweden

Funder

NASA Cassini

NASA Planetary Atmospheres

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference93 articles.

1. Deriving solar X ray irradiance from Yohkoh observations;Acton;J. Geophys. Res.,1999

2. On magnetospheric electron impact ionization and dynamics in Titan's ram-side and polar ionosphere-A Cassini case study;Agren;Ann. Geophys.,2007

3. On the ionospheric structure of Titan;Ågren;Planet. Space Sci.,2009

4. Detection of negative ions in the deep ionosphere of Titan during the Cassini T70 flyby;Ågren;Geophys. Res. Lett.,2012

5. Anicich , V. 2003 An Index of the Literature for Bimolecular Gas Phase Cation-Molecule Reaction Kinetics 1 28

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