Using global MHD simulations, we construct a 3D parametric Martian bow shock model that
employs a generalized conic section function defined by seven parameters. Effects of the …

Based on a new mathematical framework and large multi-year multi-mission data sets, we
reconstruct electric currents and magnetic fields around the dayside magnetopause and …

The Earth's dipole tilt angle changes both diurnally and seasonally and introduces
numerous variabilities in the coupled magnetosphere‐ionosphere system. By altering the …

A quantitative model of the magnetosheath (MS) magnetic structure is developed, using a
multi‐year set of Geotail, Themis, Cluster, and MMS magnetometer and plasma instrument …

The frozen-in interplanetary magnetic field (IMF) in the solar wind is one of the most
important parameters affecting the Earth's space weather. In the early studies of the IMF's …

Lunar Environment heliospheric X-ray Imager (LEXI) and Solar wind–Magnetosphere-
Ionosphere Link Explorer (SMILE) will observe magnetosheath and its boundary motion in …

Ground and space-based observations of the geomagnetic field are usually a superposition
of different sources from the Earth's core, lithosphere, ocean, ionosphere, and …

Large‐scale patterns of the steady‐state magnetosheath plasma flow and their dependence
on the interplanetary magnetic field (IMF) have been reconstructed for the first time on the …

Simulation results from a global magnetohydrodynamic (MHD) model are used to examine
whether the bow shock has an indentation and characterize its formation conditions, as well …

In studies of physical processes near planetary bow shocks, empirical models of the latter
are usually used. While computational magneto‐hydrodynamics (MHD) or kinetic models of …