output
20082026
most citedWhistler mode waves and the electron heat flux in the solar wind: Cluster observations

142 citations

Showing astro-ph.EPShow all

5 papers · 1 filter

astro-ph.EP2023★ 45 cited

Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer

Leigh N. Fletcher, Thibault Cavalié, Davide Grassi +47

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…

astro-ph.EP2022★ 17 cited

Do we need to consider electron kinetic effects to properly model a planetary magnetosphere: the case of Mercury

Giovanni Lapenta, David Schriver, Raymond J. Walker +4

The magnetosphere of Mercury is studied using an implicit full particle in cell simulation (PIC). We use a hybrid simulation where ions are full particles and electrons are conside…

astro-ph.EP2020★ 3 cited

Locating the Source Field Lines of Jovian Decametric Radio Emissions

Yuming Wang, Xianzhe Jia, Chuanbing Wang +2

Decametric (DAM) radio emissions are one of the main windows through which one can reveal and understand the Jovian magnetospheric dynamics and its interaction with the moons. DAMs…

astro-ph.EP2019★ 27 cited

Modeling Kelvin-Helmholtz instability-driven turbulence with hybrid simulations of Alfvénic turbulence

Luca Franci, Julia E. Stawarz, Emanuele Papini +9

Magnetospheric Multiscale (MMS) observations of plasma turbulence generated by a Kelvin-Helmholtz (KH) event at the Earth's magnetopause are compared with a high-resolution two-dim…

astro-ph.EP2018★ 24 cited

Supermassive Hot Jupiters Provide More Favourable Conditions for the Generation of Radio Emission via the Cyclotron Maser Instability - A Case Study Based on Tau Bootis b

C. Weber, N. V. Erkaev, V. A. Ivanov +5

We investigate under which conditions supermassive hot Jupiters can sustain source regions for radio emission, and whether this emission could propagate to an observer outside the…