Laurent Lamy

TL;DR: A large campaign of observations of these planets has been undertaken using the Hubble Space Telescope, in association with measurements from planetary spacecraft and solar wind conditions both propagated from 1 AU and measured near each planet as mentioned in this paper.

TL;DR: In this article, the average properties, and characteristics of the SKR over 2.75 years starting at Cassini's Saturn orbit insertion were analyzed based on carefully calibrated and cleaned longterm time series and dynamic spectra.

TL;DR: In this article, the authors investigated the evolution of the properties of planetary period magnetic field oscillations observed by the Cassini spacecraft in Saturn's magnetosphere over the interval from late 2004 to early 2011, spanning equinox in mid-2009.

TL;DR: The detection of magnetic-field-aligned ion and electron beams with sufficient power to stimulate detectable aurora is reported, and the subsequent discovery of Enceladus-associated aurora in a few per cent of the scans of the moon’s footprint.

TL;DR: In this article, the ionospheric response to auroral precipitation at the giant planets is reviewed, using models and observations The emission processes for aurorae at radio, infrared, visible, ultraviolet, and X-ray wavelengths are described, and exemplified using ground-and space-based observations Comparisons between the emissions at different wavelengths are made, where possible, and interpreted in terms of precipitating particle characteristics or atmospheric conditions.