Geophysical characterization of the interiors of Ganymede, Callisto and Europa by ESA's JUpiter ICy moons Explorer
Abstract The JUpiter ICy moons Explorer (JUICE) of ESA was launched on 14 April 2023
and will arrive at Jupiter and its moons in July 2031. In this review article, we describe how …
and will arrive at Jupiter and its moons in July 2031. In this review article, we describe how …
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 …
[HTML][HTML] The search for radio emission from the exoplanetary systems 55 Cancri, υ Andromedae, and τ Boötis using LOFAR beam-formed observations
JD Turner, P Zarka, JM Grießmeier, J Lazio… - Astronomy & …, 2021 - aanda.org
Context. The detection of radio emissions from exoplanets will open up a vibrant new
research field. Observing planetary auroral radio emission is the most promising method to …
research field. Observing planetary auroral radio emission is the most promising method to …
The Io, Europa, and Ganymede auroral footprints at Jupiter in the ultraviolet: Positions and equatorial lead angles
Jupiter's satellite auroral footprints are a consequence of the interaction between the Jovian
magnetic field with co‐rotating iogenic plasma and the Galilean moons. The disturbances …
magnetic field with co‐rotating iogenic plasma and the Galilean moons. The disturbances …
Hunting for exoplanets via magnetic star–planet interactions: geometrical considerations for radio emission
Recent low-frequency radio observations suggest that some nearby M dwarfs could be
interacting magnetically with undetected close-in planets, powering the emission via the …
interacting magnetically with undetected close-in planets, powering the emission via the …
Source of radio emissions induced by the Galilean moons Io, Europa and Ganymede: in situ measurements by Juno
At Jupiter, part of the auroral radio emissions are induced by the Galilean moons Io, Europa
and Ganymede. Until now, except for Ganymede, they have been only remotely detected …
and Ganymede. Until now, except for Ganymede, they have been only remotely detected …
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 …
Fine structures of radio bursts from flare star AD Leo with FAST observations
Radio bursts from nearby active M-dwarfs have been frequently reported and extensively
studied in solar or planetary paradigms. Whereas, their substructures or fine structures …
studied in solar or planetary paradigms. Whereas, their substructures or fine structures …
Radio emission from UV Cet: auroral emission from a stellar magnetosphere
TS Bastian, WD Cotton, G Hallinan - The Astrophysical Journal, 2022 - iopscience.iop.org
The archetypical flare star UV Cet was observed by MeerKAT on 2021 October 5–6. A large
radio outburst with a duration of∼ 2 hr was observed between 886 and 1682 MHz, with a …
radio outburst with a duration of∼ 2 hr was observed between 886 and 1682 MHz, with a …
Search for Jovian decametric emission induced by Europa on the extensive Nançay Decameter Array catalog
Context. The electrodynamic interaction between the Galilean satellites and the Jovian
magnetosphere generates Alfvén wings that connect the satellites to the polar atmosphere …
magnetosphere generates Alfvén wings that connect the satellites to the polar atmosphere …