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 …

Mars' crustal magnetic field holds information on the planet's interior evolution and exterior
processes that have modified the crust. Crustal magnetization records an ancient dynamo …

Abstract The Mars Atmosphere and Volatile Evolution mission has obtained comprehensive
particle and magnetic field measurements. The Solar Wind Electron Analyzer provides …

We present multi‐instrument observations of the effects of solar wind on ion escape fluxes
on Mars based on the Mars Atmosphere and Volatile EvolutioN (MAVEN) data from 1 …

We present results from a global Mars time‐dependent MHD simulation under constant solar
wind and solar radiation impact considering inherent magnetic field variations due to …

The Martian interaction with the solar wind leads to the formation of a bow shock upstream of
the planet. The shock dynamics appear complex, due to the combined influence of external …

The Martian magnetosphere contains elements of induced and intrinsic origin. To display
them one must use different coordinate systems. Although the solar‐electric coordinate …

It is important to include the effects of cold ions when we consider heavy ion outflows from
Mars. We here report on statistical properties of heavy ion outflows (including cold ion …

The first estimation of the incompressible energy cascade rate at magnetohydrodynamic
(MHD) scales in the plasma upstream of the Martian bow shock is obtained, making use of …

Abstract Based on the Mars Atmosphere and Volatile EvolutioN (MAVEN) observations, we
have analyzed the role of the crustal magnetic field on ion loss driven by the direct …