Aerosols: The key to understanding Titan's lower ionosphere. (April 2018)

• Record Type: Journal Article
• Authors: Molina-Cuberos, G.J.; Cardnell, S.; García-Collado, A.J.; Witasse, O.; López-Moreno, J.J.
• Is Part Of: Planetary and space science. Volume 153(2018)
• Page Start: 157
• Page End: 162
• Publication Date: 2018-04
• Subjects: Titan -- Comic rays -- Aerosols -- Charge concentration -- Ionosphere; Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2018.02.007
• Languages: English
• ISSNs: 0032-0633

Abstract

Abstract: The Permittivity Wave and Altimetry system on board the Huygens probe observed an ionospheric hidden layer at a much lower altitude than the main ionosphere during its descent through the atmosphere of Titan, the largest satellite of Saturn. Previous studies predicted a similar ionospheric layer. However, neither previous nor post-Huygens theoretical models have been able to reproduce the measurements of the electrical conductivity and charge densities reported by the Mutual Impedance (MI) and Relaxation Probe (RP) sensors. The measurements were made from an altitude of 140 km down to the ground and show a maximum of charge densities of ≈ 2 × 10 9 m −3 positive ions and ≈ 450 × 10 6 m −3 electrons at approximately 65 km. Such a large difference between positive and negative charge densities has not yet been understood. Here, by making use of electron and ion capture processes in to aerosols, we are able to model both electron and positive ion number densities and to reconcile experimental data and model results. Highlights: Huygens HASI plasma data explained with the help of numerical modelling. New model of the ionosphere including aerosols, based on a recent Mars model. Dependence of electrical conductivity with aerosols distribution.