Two of the primary goals of the MAVEN mission are to determine how the rate of escape of
Martian atmospheric gas to space at the current epoch depends upon solar influences and …

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 …

Coupling between the lower and upper atmosphere, combined with loss of gas from the
upper atmosphere to space, likely contributed to the thin, cold, dry atmosphere of modern …

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

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

The Martian‐induced magnetopause (IMP), characterized by the sudden changes of
magnetic fields and ion compositions, is the transition boundary separating the …

For the first time, we explore the tightly coupled interior‐magnetosphere system of Mercury
by employing a three‐dimensional ten‐moment multifluid model. This novel fluid model …

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 …

Mars lacks a global magnetic field, and instead possesses small-scale crustal magnetic
fields, making its magnetic environment fundamentally different from intrinsic …

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 …