Abstract ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …

Cyclotron resonance between plasma waves and charged particles is a fundamental and
ubiquitous process in the plasma universe, during which the particle's gyromotion has a …

The excitation of electrostatic and/or electromagnetic waves in the plasma universe is often
associated with anisotropic velocity distributions of charged particles. In Earth's inner …

Relativistic electron precipitation (REP) from the Earth's radiation belt plays an important role
in mesospheric ozone loss as a connection between space weather and the climate system …

Mars is typically regarded as a non‐magnetic planet. Currents in the Martian ionosphere
generate a Venus‐like induced magnetosphere which deflects the solar wind flow s and …

Planetary magnetic fields control energetic particles in their space environments and guide
particles to polar atmospheres, where they produce stunning auroral forms. As revealed by …

By constructing an empirical model of the spectral and latitudinal distribution of ion cyclotron
waves on the basis of Cassini datasets, we investigate the resonant interactions between …

One of the auroral features of Jupiter is the emission associated with the orbital motion of its
moon Io. The relative velocity between Io and the surrounding plasma trigger perturbations …

Repeating X-ray bursts from the Galactic magnetar SGR 1806-20 have been observed with
a period of 398 days. Similarly, periodic X-ray bursts from SGR 1935+ 2154 with a period of …

The decadal global magnetoactivity evolution profile that precedes short-burst pulses in
magnetar 4U 0142+ 61 and superhumps (superoutbursts) in dwarf novae now also emerges …