Our current knowledge of the spatial structure of the Venus ionosphere and its temporal
behavior is reviewed, with emphasis on the more recent Pioneer Venus measurements and …

We review here observations and models related to the chemical and thermal structures,
airglow and auroral emissions and dynamics of the Venus thermosphere, and compare …

Venus has been more frequently studied by space missions than any other planet.
Consequently, we know more about the solar wind interaction with Venus than with any …

The Pioneer Venus Orbiter measurements of the plasma and magnetic environment of the
near tail of Venus show that the ionosphere becomes increasingly filamentary with …

Measurements of electron density and temperature by the Pioneer Venus orbiter electron
temperature probe have been employed to examine the characteristics and morphology of …

The objective of this White Paper, submitted to ESA's Voyage 2050 call, is to get a more
holistic knowledge of the dynamics of the Martian plasma system, from its surface up to the …

The nightside Martian ionosphere is thought to be contributed by day‐to‐night transport and
electron precipitation, of which the former has not been well studied. In this work, we …

We have predicted the escape fluxes of energetic O from Mars for high and low solar activity
models of the martian thermosphere, using a Monte Carlo code to determine the escape …

Dynamics play an important role in defining the characteristics of the Venus ionosphere. The
absence of a significant internal magnetic field at Venus allows the ionization to respond …

This article reviews our understanding of the ionospheres in the solar system. It provides
some basic information on the sources and sinks of the ionospheric plasma, its dynamics …