Radio signatures of star–planet interactions, exoplanets and space weather
Radio detections of stellar systems provide a window onto stellar magnetic activity and the
space weather conditions of extrasolar planets—information that is difficult to obtain at other …
space weather conditions of extrasolar planets—information that is difficult to obtain at other …
The Radio & Plasma Wave Investigation (RPWI) for the JUpiter ICy moons Explorer (JUICE)
JE Wahlund, JES Bergman, L Åhlén, W Puccio… - Space Science …, 2025 - Springer
Abstract The Radio & Plasma Wave Investigation (RPWI) onboard the ESA JUpiter ICy
moons Explorer (JUICE) is described in detail. The RPWI provides an elaborate set of state …
moons Explorer (JUICE) is described in detail. The RPWI provides an elaborate set of state …
Drifting discrete Jovian radio bursts reveal acceleration processes related to Ganymede and the main aurora
E Mauduit, P Zarka, L Lamy, SLG Hess - Nature Communications, 2023 - nature.com
Radio detection at high time-frequency resolutions is a powerful means of remotely studying
electron acceleration processes. Radio bursts have characteristics (polarization, drift …
electron acceleration processes. Radio bursts have characteristics (polarization, drift …
Poynting fluxes, field‐aligned current densities, and the efficiency of the Io‐Jupiter electrodynamic interaction
Juno's highly inclined orbits provide opportunities to sample high‐latitude magnetic field
lines connected to the orbit of Io, among the other Galilean satellites. Its payload offers both …
lines connected to the orbit of Io, among the other Galilean satellites. Its payload offers both …
Jupiter science enabled by ESA's Jupiter icy moons explorer
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 …
Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital …
Kinetic Alfvén waves and auroral particle acceleration: A review
RL Lysak - Reviews of Modern Plasma Physics, 2023 - Springer
Shear mode Alfvén waves are the carriers of field-aligned currents in the auroral zones of
Earth and other planets. These waves travel along the magnetic field lines, coupling the …
Earth and other planets. These waves travel along the magnetic field lines, coupling the …
Electron energization by inertial Alfvén waves in density depleted flux tubes at Jupiter
Juno satellite observations have illustrated substantial examples of broadband electron
energization up to 105–106 eV levels. In order to explain these observations, we use a …
energization up to 105–106 eV levels. In order to explain these observations, we use a …
How Bi‐Modal Are Jupiter's Main Aurora Zones?
Using Juno‐measured> 30 keV electrons, three regions with substantial ultraviolet
emissions were identified previously for Jupiter's main aurora (excluding the polar cap): low …
emissions were identified previously for Jupiter's main aurora (excluding the polar cap): low …
Dawn-dusk asymmetry in the main auroral emissions at Jupiter observed with Juno-UVS
Jupiter's main auroral emissions usually form auroral curtains surrounding the magnetic
poles. Most explanations for this auroral feature are based on corotation enforcement …
poles. Most explanations for this auroral feature are based on corotation enforcement …
A unified framework for global auroral morphologies of different planets
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 …
particles to polar atmospheres, where they produce stunning auroral forms. As revealed by …