activity
20162026
most citedOn the Existence of the Kolmogorov Inertial Range in the Terrestrial Magnetosheath Turbulence

126 citations · 829 across the 25 of their papers we have counts for

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Showing 2021Show all

7 papers · 1 filter

physics.plasm-ph2021★ 27 cited

The incompressible energy cascade rate in anisotropic solar wind turbulence

N. Andrés, F. Sahraoui, Huang +2

Context. The presence of a magnetic guide field induces several types of anisotropy in solar wind turbulence. The energy cascade rate between scales in the inertial range depends s…

astro-ph.EP2021★ 1 cited

Science goals and new mission concepts for future exploration of Titan's atmosphere geology and habitability: Titan POlar Scout/orbitEr and In situ lake lander and DrONe explorer (POSEIDON)

Sébastien Rodriguez, Sandrine Vinatier, Daniel Cordier +61

In response to ESA Voyage 2050 announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn largest m…

astro-ph.EP2021★ 2 cited

Reply to comment on "An Active Plume Eruption on Europa During Galileo Flyby E26 as Indicated by Energetic Proton Depletions"

H. L. F. Huybrighs, E. Roussos, A. Blöcker +6

In Huybrighs et al., 2020 we investigated energetic proton depletions along Galileo's Europa flyby E26. Based on a particle tracing analysis we proposed that depletions are caused…

astro-ph.EP2021★ 9 cited

Re-Analysis of the Cassini RPWS/LP Data in Titan's Ionosphere: 2. Statistics on 57 Flybys

A. Chatain, J. -E. Wahlund, O. Shebanits +5

The ionosphere of Titan hosts a complex ion chemistry leading to the formation of organic dust below 1200 km. Current models cannot fully explain the observed electron temperature…

astro-ph.EP2021★ 10 cited

Re-Analysis of the Cassini RPWS/LP Data in Titan's Ionosphere: 1. Detection of Several Electron Populations

A. Chatain, J. -E. Wahlund, O. Shebanits +5

Current models of Titan ionosphere have difficulties in explaining the observed electron density and/or temperature. In order to get new insights, we re-analyzed the data taken in…

physics.space-ph2021★ 37 cited

The evolution of compressible solar wind turbulence in the inner heliosphere: PSP, THEMIS and MAVEN observations

N. Andrés, F. Sahraoui, L. Z. Hadid +5

The first computation of the compressible energy transfer rate from 0.2 AU up to 1.7 AU is obtained using PSP, THEMIS and MAVEN observations. The compressible energy…

physics.space-ph2021★ 39 cited

The Ion Transition Range of Solar Wind Turbulence in the Inner Heliosphere: Parker Solar Probe Observations

S. Y. Huang, F. Sahraoui, N. Andrés +15

The scaling of the turbulent spectra provides a key measurement that allows to discriminate between different theoretical predictions of turbulence. In the solar wind, this has dri…