Both heliophysics and planetary physics seek to understand the complex nature of the solar
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …

Abstract Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) is a novel self-
standing mission dedicated to observing the solar wind–magnetosphere coupling via …

Plasma convection on a global scale is a fundamental feature of planetary magnetosphere.
The Dungey cycle explains that steady-state convection within the closed part of the …

In Earth's low atmosphere, hurricanes are destructive due to their great size, strong spiral
winds with shears, and intense rain/precipitation. However, disturbances resembling …

The impact of geomagnetically induced currents (GICs) on the power networks at middle
and low latitudes has attracted attention in recent years with the increase of large‐scale …

Saturn's magnetospheric structure and the intensity of radio frequency emissions from its
immediate surroundings are modulated at close to the planet's rotation period. Analogous …

We investigate the solar wind interaction with Saturn's magnetosphere by using a global
magnetohydrodynamic simulation driven by an idealized time‐varying solar wind input that …

Dynamics of the near‐Earth magnetotail associated with substorms during a period of
extended southward interplanetary magnetic field is studied using a three‐dimensional (3 …

Imaging is one of the essential techniques to observe astronomical structures. While
analyzing the observed images, it is a challenge in many scientific fields to reconstruct the 3 …

A distinct class of aurora, called transpolar auroral arc (TPA)(in some cases called “theta”
aurora), appears in the extremely high-latitude ionosphere of the Earth when interplanetary …