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 …

The solar wind interaction with Mars controls the transfer of energy and momentum from the
solar wind into the magnetosphere, ionosphere and atmosphere, driving structure, and …

Ion escape to space through the interaction of solar wind and Mars is an important factor
influencing the evolution of the Martian atmosphere. The plasma clouds (explosive bulk …

This study presents a new spherical harmonic (SH) model of the crustal magnetic field of
Mars, based on the magnetic field data set measured by the Mars Global Surveyor (MGS) …

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

Ion escape from the atmosphere to space is one of the most likely reasons to account for the
evolution of the Martian climate. Based on three-dimensional multifluid …

The Martian bow shock (BS) is generated with the mass-loading and magnetic pileup
processes when the solar wind interacts with the Martian ionosphere. In this vein, the …

Using global magnetohydrodynamic simulations, we construct a 3D parametric model of the
Martian magnetic pileup boundary (MPB). This model employs a modified parabola function …

In the Martian induced magnetosphere, the motion of planetary ions is significantly
controlled by the ambient electric fields, which can be decomposed into three components …

We study the solar wind interaction with Mars in a global three‐dimensional hybrid model. A
well‐developed, vast ion foreshock forms under a strongly flow‐aligned interplanetary …