Title
Energy deposition and ion production from thermal oxygen ion precipitation during Cassini’s T57 flyby
Document Type
Article
Department or Administrative Unit
Physics
Publication Date
5-1-2018
Abstract
Cassini’s Radio Science Investigation (RSS) and Langmuir Probe observed abnormally high electron densities in Titan’s ionosphere during Cassini’s T57 flyby. We have developed a three-dimensional model to investigate how the precipitation of thermal magnetospheric O+ may have contributed to enhanced ion production in Titan’s ionosphere. The three-dimensional model builds on previous work because it calculates both the flux of oxygen through Titan’s exobase and the energy deposition and ion production rates in Titan’s atmosphere. We find that energy deposition rates and ion production rates due to thermal O+ precipitation have a similar magnitude to the rates from magnetospheric electron precipitation and that the simulated ionization rates are sufficient to explain the abnormally high electron densities observed by RSS and Cassini’s Langmuir Probe. Globally, thermal O+ deposits less energy in Titan’s atmosphere than solar EUV, suggesting it has a smaller impact on the thermal structure of Titan’s neutral atmosphere. However, our results indicate that thermal O+ precipitation can have a significant impact on Titan’s ionosphere.
Recommended Citation
Snowden, D., Smith, M., Jimson, T., & Higgins, A. (2018). Energy deposition and ion production from thermal oxygen ion precipitation during Cassini’s T57 flyby. Icarus, 305, 186–197. https://doi.org/10.1016/j.icarus.2018.01.014
Journal
Icarus
Rights
© 2018 Elsevier Inc. All rights reserved.
Comments
This article was originally published in Icarus. The full-text article from the publisher can be found here.
Due to copyright restrictions, this article is not available for free download from ScholarWorks @ CWU.