activity
20072020
most citedSmall Scale Energy Cascade of the Solar Wind Turbulence

267 citations · 779 across the 11 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2020

Coherent events at ion scales in the inner Heliosphere: \textit{Parker Solar Probe} observations during the first Encounter

Denise Perrone, Roberto Bruno, Raffaella D'Amicis +7

\textit{Parker Solar Probe} has shown the ubiquitous presence of strong magnetic field deflections, namely switchbacks, during its first perihelion where it was embedded in a highl…

astro-ph.SR2020112 cited

The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

I. Zouganelis, A. De Groof, A. P. Walsh +182

Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, from a close distance, in and out of the ecliptic. The ultimate goal is to understand…

physics.space-ph2020

Magnetic field turbulence in the solar wind at sub-ion scales: in situ observations and numerical simulations

L. Matteini, L. Franci, O. Alexandrova +5

We investigate the transition of the solar wind turbulent cascade from MHD to sub-ion range by means of a detail comparison between in situ observations and hybrid numerical simula…

physics.space-ph202030 cited

Whistler Waves and Electron Properties in the Inner Heliosphere: Helios Observations

Vamsee Krishna Jagarlamudi, Olga Alexandrova, Laura Bercic +4

We present the analysis of narrowband whistler wave signatures observed in the inner heliosphere (0.3-1 au). These signatures are bumps in the spectral density in the 10-200 Hz fre…

physics.space-ph202025 cited

Observational quantification of three-dimensional anisotropies and scalings of space plasma turbulence at kinetic scales

Tieyan Wang, Jiansen He, Olga Alexandrova +2

A statistical survey of spectral anisotropy of space plasma turbulence is performed using five years measurements from MMS in the magnetosheath. By measuring the five-point second-…

physics.space-ph2020

Kinetic turbulence in space plasmas observed in the near-Earth and near-Sun solar wind

Olga Alexandrova, Vamsee Krishna Jagarlamudi, Claudia Rossi +4

Turbulence develops in any stressed flow when the scales of the forcing are much larger than those of the dissipation. In neutral fluids, it consists of chaotic motions in physical…