Venus has intrigued planetary scientists for decades because of its huge contrasts to Earth,
in spite of its nickname of “Earth's Twin”. Its invisible upper atmosphere and space …

This article summarizes and aims at comparing the main features of the induced
magnetospheres of Mars, Venus and Titan. All three objects form a well-defined induced …

This textbook, derived from courses given by three leading researchers, provides advanced
undergraduates and graduates with up-to-date coverage of space physics, from the Sun to …

Using over 6 years of magnetic field data (October 2014–December 2020) collected by the
Mars Atmosphere and Volatile EvolutioN, we conduct a statistical study on the three …

Observations with the Venus Express magnetometer and low-energy particle detector
revealed magnetic field and plasma behavior in the near-Venus wake that is symptomatic of …

We utilize suprathermal ion and magnetic field measurements from the Mars Atmosphere
and Volatile EvolutioN (MAVEN) mission, organized by the upstream magnetic field, to …

Abstract Analysis of Mars Atmosphere and Volatile Evolution (MAVEN)/Supra‐Thermal And
Thermal Ion Composition observations in the Martian upper atmosphere, bounded at higher …

The correlation between space environment conditions and the properties of escaping ions
is a central topic of Mars research. Although empirical correlations have been visible in the …

The present atmosphere of Venus contains almost no water, but recent measurements
indicate that in its early history, Venus had an Earth‐like ocean. Understanding how the …

A fundamental question for the atmospheric evolution of Venus is how much water‐related
material escapes from Venus to space. In this study, we calculate the nonthermal escape of …