The upper atmospheres of unmagnetized solar system bodies interact more directly with
their local plasma environment than their counterparts on magnetized bodies such as Earth …

Ionospheres provides a comprehensive description of the physical, plasma and chemical
processes controlling the behavior of ionospheres. The relevant transport equations and …

The formation of Titan's induced magnetosphere is a unique and important example in the
solar system of a plasma-moon interaction where the moon has a substantial atmosphere …

Aeronomy is a description of the physics and chemistry of the upper atmospheres and
ionospheres of planetary bodies. In this chapter we consider those processes occurring in …

Simulation has become a valuable tool that compliments more traditional methods used to
understand solar system plasmas and their interactions with planets, moons and comets …

We study the interaction between the atmospheres of Venus-like, non-magnetized
exoplanets orbiting an M-dwarf star, and the stellar wind using a multi-species MHD model …

Titan, SATURN's largest satellite, is a distant world: far away from the Sun and its close,
warm TERRESTRIAL PLANETS. A fair distance from Saturn, too. Seen from Titan, at more …

The long‐term statistical behavior of the large‐scale structure of Saturn's magnetosphere
has been investigated. Established statistical techniques for Jupiter have been applied to …

Electromagnetic induction is a powerful technique to study the electrical conductivity of the
interior of the Earth and other solar system bodies. Information about the electrical …

The Cassini Ion Neutral Mass Spectrometer (INMS) has measured both neutral and ion
species in Titan's upper atmosphere and ionosphere and the Enceladus plumes. Ion …